ABSTRACT
We report a comprehensive list of accurate Ritz wavelengths for parity-forbidden [Co ii] and [V ii] lines obtained from the analysis of energy levels measured in the laboratory with Fourier transform emission spectroscopy. Such lines, particularly those in the infrared, are in demand for the analysis of low-density astrophysical plasmas in and around objects such as planetary nebulae, star-forming regions, and active galactic nuclei. Transitions between all known metastable levels of Co ii and V ii are included in our analysis, producing wavelengths for 1477 [V ii] lines and 782 [Co ii] lines. Of these, 170 [V ii] lines and 171 [Co ii] lines arise from transitions with calculated transition probabilities greater than 1 × 10−2 s−1 and upper level excitations of less than 5 eV, and thus are likely to be observed in astrophysical spectra.
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1. INTRODUCTION
Stellar spectra feature a rich array of absorption lines, generated primarily from electric dipole (E1) transitions within the atoms of a star's atmosphere. These lines may be interpreted using synthetic spectra derived from atomic and molecular line lists, and radiative processes modeled using spectra containing hundreds of millions or billions of spectroscopic transitions.
In each case though, fundamental atomic data—such as line wavelengths and identifications, transition probabilities, and line broadening parameters such as hyperfine splitting—must be known. These can be supplied on a large scale through ab initio atomic and molecular calculations, or with greater accuracy on a smaller scale through direct experimental measurements in the laboratory.
However, in recent decades, developments in astronomical spectrographs have placed greater demands on the quantity and accuracy of such data. As a result, our understanding of stellar atmospheres is frequently not limited by the quality and quantity of astronomical spectra, but by the availability of accurate atomic and molecular data with which to analyze them. This is also true of other areas of astronomical spectroscopy, which may have additional, sometimes unique, requirements.
In contrast to stellar spectra, spectra from low-density astrophysical plasmas—such as those that exist in planetary nebulae and star-forming regions, and around active galactic nuclei—also contain strong emission lines. These are generated through a number of processes, and can lead to the observation of so-called forbidden lines, which arise from the radiative de-excitation of electrons from long-lived, low-lying metastable levels. For an overview of the processes at work in nebulae and active galactic nuclei, see Osterbrock & Ferland (2006), for example.
In general, metastable levels possess the same parity as the ground state of an atom,1 and are of lower energy than any level of opposite parity. De-excitation of electrons through E1 transitions is thus forbidden, as can be seen from the selection rules in Table 1. Electrons populating these levels must therefore de-excite through alternative mechanisms.
Table 1. Transition Rules for Allowed E1 Transitions and Parity-forbidden M1 and E2 Transitions
Transition | Parity | ΔJ | Restrictions |
---|---|---|---|
E1 | Changes | 0, ±1 | (0↮0) |
M1 | No change | 0, ±1 | (0↮0) |
E2 | No change | 0, ±1, ±2 | (0↮0, 1/2↮1/2, 0↮1) |
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Higher order, magnetic dipole (M1) and electric quadrupole (E2) transitions are allowed, but for neutral and weakly ionized atoms, their transition probabilities are many orders of magnitude smaller than those for E1 transitions. As a result, in high-density plasmas—such as those that exist in stellar atmospheres or plasmas generated in the laboratory—metastable levels are predominantly de-populated through collisions with other atoms, and thus no forbidden lines are seen. However, in low-density plasmas, collisions are rare, allowing enough time for M1 and E2 transitions to occur.
Forbidden lines are thus observed in these plasmas and are important in examining different regions of planetary nebulae (Smith et al. 2005, for example) and nebulae surrounding objects such as active galactic nuclei (Meijerink et al. 2007, for example). However, it is usual for only standard pairs of forbidden lines to be used in such analyses, most commonly those from [Fe ii], which is at least in part due to a lack of accurate atomic data for other forbidden lines. Barlow (2012) recently reviewed developments arising from spectroscopic studies of ionized nebulae and concluded that there is an "urgent" requirement for more atomic data of such lines; particularly so for atoms in low ionization states.
In this paper, we present a comprehensive set of accurate Ritz wavelengths for forbidden lines in Co ii and V ii, calculated, in each case, for transitions between all known metastable levels. These include infrared lines of astrophysical importance, some of which have already been observed in such spectra; see Fang & Liu (2011), Hartman et al. (2004), and Arkhipova et al. (2001), for example.
2. LABORATORY DATA
The Ritz wavelengths of the parity-forbidden [Co ii] and [V ii] lines reported here were calculated, respectively, from the accurate Co ii energy levels reported by Pickering et al. (1998) and the revised accurate V ii energy levels measured by Thorne et al. (2013).
In both cases, the laboratory Co ii and V ii spectra obtained by those researchers, and used in their spectral analyses, were generated in a water-cooled hollow cathode discharge lamp and measured on both the f/25 vacuum UV Fourier transform (FT) spectrometer at Imperial College London (Thorne et al. 1987) and the f/55 IR-visible FT spectrometer at the National Solar Observatory, Kitt Peak, Tucson, AZ (Brault 1976). Observed atomic lines were fitted using the GREMLIN program developed by J. W. Brault (unpublished), with care taken to account for hyperfine structure splitting by calculating a center of gravity wavenumber for each transition. The wavenumber scale was calibrated using the 26 Ar ii lines recommended by Learner & Thorne (1988), and the ELCALC program (Radziemski & Kaufman 1969) was then used to revise the energy levels involving known transitions observed in the FT spectra. New energy levels were found using the unidentified observed lines.
The Co ii spectra in Pickering et al. (1998) were wavelength calibrated using the Ar ii measurements of Norlén (1973). By contrast, the V ii spectra in Thorne et al. (2013) were wavelength calibrated using the more recent Ar ii measurements of Whaling et al. (1995). Since the measurements of Norlén (1973) have now been superseded by those of Whaling et al. (1995), we increased the Co ii energy levels of Pickering et al. (1998) by 7 parts in 108—the value recommended by Whaling et al. (1995)—in our calculations of [Co ii] Ritz wavelengths to account for the difference between the two calibration scales. In almost all cases, however, the resulting change in line wavelength was smaller than the overall wavelength uncertainty.
3. ANALYSIS AND RESULTS
3.1. Ritz Wavelengths
V ii has a complex energy level structure, with 65 metastable levels of even parity between the 3d4 a5D0 ground state and the lowest-lying level of odd parity; the 3d3(4F)4p z5G2 level at 34592.843(1) cm−1 (Thorne et al. 2013). These levels are shown in Figure 1, grouped by their configuration and sub-configuration, with individual spin-orbit (LS) terms labeled. The levels belonging to the lowest-lying term of odd parity are also shown to indicate the upper limit on the region in which E1 transitions are forbidden.
Using the energy levels measured by Thorne et al. (2013) and the selection rules given in Table 1, we calculated accurate Ritz wavelengths for the 1477 possible parity-forbidden [V ii] lines originating from M1 and E2 transitions between all 65 metastable levels. The most significant of these—those with A ⩾ 1 × 10−2 and upper level excitation of less than 5 eV—are listed in Table 2, with the remaining weaker lines listed in Table 4. The uncertainties in line wavelength were obtained by combining the uncertainty in the energy level value (typically 0.001 cm−1 to 0.003 cm−1) of each of the two levels involved in a given transition.
Table 2. Parity-forbidden Lines in V ii with a Transition Probability of At Least 1 × 10−2 s−1 and Upper Level Excitation Less Than 5 eV
Wavenumber | Unc. | λvac | Unc. | λair | Transition | Energy (cm−1)b | A | Type | ||
---|---|---|---|---|---|---|---|---|---|---|
(cm−1) | (cm−1) | (Å) | (Å) | (Å)a | Lower | Upper | Lower | Upper | (s−1)c | |
Level | Level | Level | Level | |||||||
5391.151 | 0.004 | 18548.9147 | 0.0124 | 18543.8509 | a5P3 | b3P2 | 13742 | 19133 | 1.71 × 10−2 | M1, E2 |
5649.623 | 0.004 | 17700.2961 | 0.0113 | 17695.4632 | a5P1 | b3P0 | 13512 | 19161 | 2.87 × 10−2 | M1 |
5654.515 | 0.004 | 17684.9827 | 0.0113 | 17680.1540 | a5P1 | b3P1 | 13512 | 19166 | 2.22 × 10−2 | M1, E2 |
7253.161 | 0.004 | 13787.0923 | 0.0069 | 13783.3234 | a3P2 | b3P0 | 11908 | 19161 | 1.02 × 10−2 | E2 |
7657.257 | 0.002 | 13059.5068 | 0.0038 | 13055.9357 | a3H6 | b3H6 | 12706 | 20363 | 1.99 × 10−2 | M1, E2 |
7658.766 | 0.003 | 13056.9337 | 0.0054 | 13053.3633 | a3H5 | b3H5 | 12621 | 20280 | 1.77 × 10−2 | M1, E2 |
7697.282 | 0.004 | 12991.5989 | 0.0061 | 12988.0461 | a3H4 | b3H4 | 12545 | 20242 | 1.83 × 10−2 | M1, E2 |
8387.824 | 0.004 | 11922.0432 | 0.0064 | 11918.7809 | a3P1 | a1S0 | 11515 | 19903 | 2.41 × 10−2 | M1 |
9037.817 | 0.004 | 11064.6188 | 0.0044 | 11061.5892 | b1D2 | b1F3 | 25191 | 34229 | 3.38 × 10−2 | M1, E2 |
9255.938 | 0.002 | 10803.8753 | 0.0026 | 10800.9164 | a3F4 | a3D3 | 9098 | 18354 | 2.05 × 10−2 | M1, E2 |
9427.464 | 0.003 | 10607.3065 | 0.0036 | 10604.4009 | a3F3 | a3D1 | 8842 | 18270 | 1.13 × 10−2 | E2 |
9629.152 | 0.004 | 10385.1305 | 0.0039 | 10382.2852 | a3F2 | a3D1 | 8640 | 18270 | 1.25 × 10−2 | M1, E2 |
9695.545 | 0.004 | 10314.0154 | 0.0045 | 10311.1893 | b3D3 | c3F4 | 20623 | 30319 | 1.25 × 10−2 | M1, E2 |
9955.193 | 0.004 | 10045.0087 | 0.0036 | 10042.2555 | b3H6 | c3F4 | 20363 | 30319 | 2.92 × 10−2 | E2 |
10015.040 | 0.001 | 9984.9826 | 0.0014 | 9982.2457 | a3F4 | b1G4 | 9098 | 19113 | 1.71 × 10−2 | M1, E2 |
10025.129 | 0.006 | 9974.9340 | 0.0058 | 9972.1998 | b3H4 | c3F2 | 20242 | 30268 | 3.26 × 10−2 | E2 |
10026.138 | 0.004 | 9973.9301 | 0.0042 | 9971.1963 | b3H5 | c3F3 | 20280 | 30306 | 3.11 × 10−2 | E2 |
10270.864 | 0.004 | 9736.2792 | 0.0034 | 9733.6098 | c3P2 | d3F4 | 20343 | 30614 | 1.27 × 10−2 | E2 |
10270.879 | 0.001 | 9736.2650 | 0.0013 | 9733.5955 | a3F3 | b1G4 | 8842 | 19113 | 1.04 × 10−2 | M1, E2 |
10521.060 | 0.004 | 9504.7457 | 0.0033 | 9502.1389 | a3F2 | b3P0 | 8640 | 19161 | 1.18 × 10−2 | E2 |
10525.952 | 0.004 | 9500.3283 | 0.0033 | 9497.7227 | a3F2 | b3P1 | 8640 | 19166 | 1.23 × 10−2 | M1, E2 |
10578.674 | 0.003 | 9452.9806 | 0.0025 | 9450.3878 | a5F5 | a5P3 | 3163 | 13742 | 1.85 × 10−2 | E2 |
10583.438 | 0.005 | 9448.7255 | 0.0048 | 9446.1338 | c3P1 | d3F2 | 20090 | 30673 | 1.16 × 10−2 | M1, E2 |
10626.334 | 0.004 | 9410.5832 | 0.0037 | 9408.0019 | a5F4 | a5P2 | 2968 | 13595 | 1.19 × 10−2 | E2 |
10785.764 | 0.004 | 9271.4804 | 0.0035 | 9268.9368 | a5F3 | a5P2 | 2809 | 13595 | 1.08 × 10−2 | M1, E2 |
10824.591 | 0.002 | 9238.2243 | 0.0019 | 9235.6897 | a5F2 | a5P1 | 2687 | 13512 | 1.23 × 10−2 | M1, E2 |
10837.702 | 0.003 | 9227.0483 | 0.0024 | 9224.5167 | a1H5 | b1F3 | 23391 | 34229 | 5.30 × 10−2 | E2 |
10906.759 | 0.002 | 9168.6265 | 0.0019 | 9166.1108 | a5F1 | a5P1 | 2605 | 13512 | 1.15 × 10−2 | M1, E2 |
11245.157 | 0.002 | 8892.7171 | 0.0018 | 8890.2760 | a3F4 | c3P2 | 9098 | 20343 | 1.81 × 10−2 | E2 |
11247.600 | 0.002 | 8890.7856 | 0.0018 | 8888.3450 | a3F3 | c3P1 | 8842 | 20090 | 1.56 × 10−2 | E2 |
11259.411 | 0.005 | 8881.4593 | 0.0042 | 8879.0212 | a5D1 | a3P0 | 36 | 11296 | 1.93 × 10−2 | M1 |
11318.330 | 0.007 | 8835.2257 | 0.0052 | 8832.8001 | a1D2 | d3P1 | 20981 | 32299 | 1.84 × 10−2 | M1, E2 |
11408.141 | 0.002 | 8765.6701 | 0.0017 | 8763.2633 | a5D2 | a3P1 | 107 | 11515 | 1.52 × 10−2 | M1, E2 |
11417.652 | 0.006 | 8758.3682 | 0.0045 | 8755.9634 | b3D3 | d3P2 | 20623 | 32041 | 6.46 × 10−2 | M1, E2 |
11439.123 | 0.010 | 8741.9289 | 0.0080 | 8739.5286 | a1D2 | d3P0 | 20981 | 32420 | 7.03 × 10−2 | E2 |
11449.288 | 0.003 | 8734.1676 | 0.0022 | 8731.7694 | a3F2 | c3P1 | 8640 | 20090 | 2.17 × 10−2 | M1, E2 |
11475.453 | 0.004 | 8714.2529 | 0.0032 | 8711.8601 | b3P1 | d3F3 | 19166 | 30642 | 1.44 × 10−2 | E2 |
11481.119 | 0.004 | 8709.9524 | 0.0032 | 8707.5607 | b3P2 | d3F4 | 19133 | 30614 | 2.58 × 10−2 | E2 |
11492.641 | 0.002 | 8701.2202 | 0.0017 | 8698.8309 | a5F5 | a3G5 | 3163 | 14656 | 1.37 × 10−2 | M1, E2 |
11500.996 | 0.002 | 8694.8991 | 0.0017 | 8692.5115 | a3F3 | c3P2 | 8842 | 20343 | 1.60 × 10−2 | M1, E2 |
11516.308 | 0.004 | 8683.3384 | 0.0027 | 8680.9540 | a3F2 | c3P0 | 8640 | 20157 | 3.74 × 10−2 | E2 |
11525.094 | 0.003 | 8676.7188 | 0.0024 | 8674.3361 | a3F4 | b3D3 | 9098 | 20623 | 1.60 × 10−2 | M1, E2 |
11648.390 | 0.003 | 8584.8774 | 0.0023 | 8582.5195 | b3F3 | b1D2 | 13543 | 25191 | 1.08 × 10−2 | M1, E2 |
11676.274 | 0.007 | 8564.3759 | 0.0049 | 8562.0236 | b3D3 | d3P1 | 20623 | 32299 | 5.62 × 10−2 | E2 |
11680.097 | 0.004 | 8561.5727 | 0.0030 | 8559.2212 | a3F3 | b3D1 | 8842 | 20522 | 1.51 × 10−2 | E2 |
11682.184 | 0.007 | 8560.0432 | 0.0049 | 8557.6921 | b3D2 | d3P1 | 20617 | 32299 | 4.01 × 10−2 | M1, E2 |
11697.589 | 0.005 | 8548.7702 | 0.0039 | 8546.4221 | c3P2 | d3P2 | 20343 | 32041 | 1.11 × 10−1 | M1, E2 |
11699.471 | 0.002 | 8547.3950 | 0.0016 | 8545.0473 | a5D3 | a3P2 | 209 | 11908 | 1.10 × 10−2 | M1, E2 |
11777.110 | 0.007 | 8491.0475 | 0.0052 | 8488.7150 | b3D1 | d3P1 | 20522 | 32299 | 9.32 × 10−2 | M1, E2 |
11802.977 | 0.010 | 8472.4388 | 0.0075 | 8470.1113 | b3D2 | d3P0 | 20617 | 32420 | 1.78 × 10−1 | E2 |
11881.785 | 0.004 | 8416.2439 | 0.0032 | 8413.9316 | a3F2 | b3D1 | 8640 | 20522 | 1.15 × 10−2 | M1, E2 |
11883.965 | 0.006 | 8414.7000 | 0.0041 | 8412.3881 | c3P0 | d3P2 | 20157 | 32041 | 3.83 × 10−2 | E2 |
11950.985 | 0.005 | 8367.5111 | 0.0038 | 8365.2120 | c3P1 | d3P2 | 20090 | 32041 | 1.06 × 10−1 | M1, E2 |
11956.211 | 0.006 | 8363.8537 | 0.0044 | 8361.5556 | c3P2 | d3P1 | 20343 | 32299 | 1.12 × 10−1 | M1, E2 |
12077.004 | 0.010 | 8280.1993 | 0.0070 | 8277.9238 | c3P2 | d3P0 | 20343 | 32420 | 8.69 × 10−2 | E2 |
12138.877 | 0.003 | 8237.9943 | 0.0021 | 8235.7303 | a3F3 | a1D2 | 8842 | 20981 | 1.86 × 10−2 | M1, E2 |
12209.607 | 0.006 | 8190.2718 | 0.0042 | 8188.0206 | c3P1 | d3P1 | 20090 | 32299 | 2.54 × 10−2 | M1, E2 |
12260.083 | 0.004 | 8156.5516 | 0.0024 | 8154.3096 | a3D3 | d3F4 | 18354 | 30614 | 2.25 × 10−2 | M1, E2 |
12340.565 | 0.004 | 8103.3567 | 0.0024 | 8101.1290 | a3F2 | a1D2 | 8640 | 20981 | 2.01 × 10−2 | M1, E2 |
12347.896 | 0.004 | 8098.5457 | 0.0024 | 8096.3193 | a3D2 | d3F3 | 18294 | 30642 | 1.65 × 10−2 | M1, E2 |
12379.217 | 0.005 | 8078.0553 | 0.0035 | 8075.8345 | a3D2 | d3F2 | 18294 | 30673 | 1.14 × 10−2 | M1, E2 |
12403.574 | 0.006 | 8062.1924 | 0.0038 | 8059.9758 | a3D1 | d3F2 | 18270 | 30673 | 1.72 × 10−2 | M1, E2 |
12874.321 | 0.006 | 7767.3999 | 0.0035 | 7765.2629 | b3P1 | d3P2 | 19166 | 32041 | 1.47 × 10−2 | M1, E2 |
12907.844 | 0.006 | 7747.2272 | 0.0035 | 7745.0956 | b3P2 | d3P2 | 19133 | 32041 | 1.92 × 10−2 | M1, E2 |
13255.598 | 0.004 | 7543.9825 | 0.0023 | 7541.9058 | a5D4 | a5P2 | 339 | 13595 | 1.85 × 10−1 | E2 |
13269.814 | 0.001 | 7535.9007 | 0.0008 | 7533.8261 | a5D4 | b3F4 | 339 | 13609 | 1.31 × 10−2 | M1, E2 |
13287.259 | 0.010 | 7526.0067 | 0.0059 | 7523.9348 | b3P2 | d3P0 | 19133 | 32420 | 1.91 × 10−2 | E2 |
13303.009 | 0.002 | 7517.0963 | 0.0013 | 7515.0269 | a5D3 | a5P1 | 209 | 13512 | 2.21 × 10−1 | E2 |
13370.017 | 0.003 | 7479.4221 | 0.0016 | 7477.4245 | a5F5 | b3G5 | 3163 | 16533 | 2.88 × 10−2 | M1, E2 |
13402.515 | 0.002 | 7461.2862 | 0.0012 | 7459.2934 | a5D4 | a5P3 | 339 | 13742 | 1.76 × 10−1 | M1, E2 |
13405.156 | 0.002 | 7459.8162 | 0.0012 | 7457.8238 | a5D2 | a5P1 | 107 | 13512 | 1.43 × 10−1 | M1, E2 |
13453.139 | 0.001 | 7433.2095 | 0.0008 | 7431.2240 | a5F4 | b3G4 | 2968 | 16422 | 1.57 × 10−2 | M1, E2 |
13475.697 | 0.003 | 7420.7664 | 0.0016 | 7418.7842 | a5D1 | a5P1 | 36 | 13512 | 3.79 × 10−2 | M1, E2 |
13488.080 | 0.004 | 7413.9537 | 0.0023 | 7411.9732 | a5D2 | a5P2 | 107 | 13595 | 6.33 × 10−2 | M1, E2 |
13532.850 | 0.002 | 7389.4265 | 0.0012 | 7387.4525 | a5D3 | a5P3 | 209 | 13742 | 1.55 × 10−1 | M1, E2 |
13558.621 | 0.004 | 7375.3813 | 0.0024 | 7373.4110 | a5D1 | a5P2 | 36 | 13595 | 1.08 × 10−1 | M1, E2 |
13594.723 | 0.005 | 7355.7953 | 0.0027 | 7353.8301 | a5D0 | a5P2 | 0 | 13595 | 5.27 × 10−2 | E2 |
13634.997 | 0.002 | 7334.0684 | 0.0012 | 7332.1088 | a5D2 | a5P3 | 107 | 13742 | 7.67 × 10−2 | M1, E2 |
13686.808 | 0.005 | 7306.3055 | 0.0029 | 7304.3532 | a3D3 | d3P2 | 18354 | 32041 | 6.92 × 10−2 | M1, E2 |
13705.538 | 0.003 | 7296.3207 | 0.0015 | 7294.3710 | a5D1 | a5P3 | 36 | 13742 | 1.83 × 10−2 | E2 |
13746.764 | 0.005 | 7274.4393 | 0.0028 | 7272.4953 | a3D2 | d3P2 | 18294 | 32041 | 1.34 × 10−2 | M1, E2 |
13785.545 | 0.004 | 7253.9751 | 0.0019 | 7252.0365 | b3G5 | c3F4 | 16533 | 30319 | 8.54 × 10−2 | M1, E2 |
13884.861 | 0.003 | 7202.0887 | 0.0016 | 7200.1636 | b3G4 | c3F3 | 16422 | 30306 | 5.58 × 10−2 | M1, E2 |
13897.000 | 0.003 | 7195.7977 | 0.0016 | 7193.8743 | b3G4 | c3F4 | 16422 | 30319 | 1.38 × 10−2 | M1, E2 |
13926.530 | 0.005 | 7180.5396 | 0.0028 | 7178.6202 | b3G3 | c3F2 | 16341 | 30268 | 4.80 × 10−2 | M1, E2 |
13945.430 | 0.006 | 7170.8079 | 0.0033 | 7168.8911 | a3D3 | d3P1 | 18354 | 32299 | 5.96 × 10−2 | E2 |
13965.408 | 0.004 | 7160.5498 | 0.0018 | 7158.6357 | b3G3 | c3F3 | 16341 | 30306 | 1.28 × 10−2 | M1, E2 |
14005.386 | 0.006 | 7140.1102 | 0.0032 | 7138.2014 | a3D2 | d3P1 | 18294 | 32299 | 1.95 × 10−2 | M1, E2 |
14029.743 | 0.007 | 7127.7143 | 0.0034 | 7125.8087 | a3D1 | d3P1 | 18270 | 32299 | 5.60 × 10−2 | M1, E2 |
14080.927 | 0.004 | 7101.8052 | 0.0018 | 7099.9063 | b3G5 | d3F4 | 16533 | 30614 | 1.72 × 10−1 | M1, E2 |
14108.784 | 0.004 | 7087.7830 | 0.0018 | 7085.8879 | b3G5 | d3F3 | 16533 | 30642 | 3.20 × 10−2 | E2 |
14126.179 | 0.010 | 7079.0551 | 0.0051 | 7077.1622 | a3D2 | d3P0 | 18294 | 32420 | 1.18 × 10−1 | E2 |
14192.382 | 0.003 | 7046.0336 | 0.0016 | 7044.1493 | b3G4 | d3F4 | 16422 | 30614 | 3.72 × 10−2 | M1, E2 |
14220.239 | 0.003 | 7032.2306 | 0.0016 | 7030.3500 | b3G4 | d3F3 | 16422 | 30642 | 1.69 × 10−1 | M1, E2 |
14251.560 | 0.005 | 7016.7757 | 0.0025 | 7014.8991 | b3G4 | d3F2 | 16422 | 30673 | 4.87 × 10−2 | E2 |
14300.786 | 0.004 | 6992.6226 | 0.0018 | 6990.7523 | b3G3 | d3F3 | 16341 | 30642 | 5.43 × 10−2 | M1, E2 |
14332.107 | 0.005 | 6977.3412 | 0.0026 | 6975.4748 | b3G3 | d3F2 | 16341 | 30673 | 2.44 × 10−1 | M1, E2 |
15115.923 | 0.002 | 6615.5404 | 0.0010 | 6613.7685 | b1G4 | b1F3 | 19113 | 34229 | 5.66 × 10−2 | M1, E2 |
15385.438 | 0.002 | 6499.6525 | 0.0009 | 6497.9108 | a5F4 | a3D3 | 2968 | 18354 | 1.81 × 10−2 | M1, E2 |
15484.912 | 0.002 | 6457.8991 | 0.0009 | 6456.1683 | a5F3 | a3D2 | 2809 | 18294 | 2.64 × 10−2 | M1, E2 |
15582.306 | 0.003 | 6417.5354 | 0.0013 | 6415.8151 | a5F2 | a3D1 | 2687 | 18270 | 2.83 × 10−2 | M1, E2 |
15662.921 | 0.003 | 6384.5052 | 0.0013 | 6382.7935 | a3G5 | c3F4 | 14656 | 30319 | 1.12 × 10−2 | M1, E2 |
15664.474 | 0.003 | 6383.8722 | 0.0013 | 6382.1607 | a5F1 | a3D1 | 2605 | 18270 | 1.48 × 10−2 | M1, E2 |
15750.321 | 0.003 | 6349.0769 | 0.0013 | 6347.3745 | a3G4 | c3F3 | 14556 | 30306 | 1.63 × 10−2 | M1, E2 |
15805.763 | 0.005 | 6326.8062 | 0.0022 | 6325.1096 | a3G3 | c3F2 | 14462 | 30268 | 4.31 × 10−2 | M1, E2 |
15844.641 | 0.004 | 6311.2822 | 0.0014 | 6309.5895 | a3G3 | c3F3 | 14462 | 30306 | 1.40 × 10−2 | M1, E2 |
15958.303 | 0.003 | 6266.3304 | 0.0012 | 6264.6495 | a3G5 | d3F4 | 14656 | 30614 | 4.19 × 10−1 | M1, E2 |
15986.160 | 0.003 | 6255.4109 | 0.0012 | 6253.7329 | a3G5 | d3F3 | 14656 | 30642 | 7.37 × 10−2 | E2 |
16057.842 | 0.003 | 6227.4869 | 0.0012 | 6225.8161 | a3G4 | d3F4 | 14556 | 30614 | 7.60 × 10−2 | M1, E2 |
16085.699 | 0.003 | 6216.7022 | 0.0012 | 6215.0342 | a3G4 | d3F3 | 14556 | 30642 | 3.20 × 10−1 | M1, E2 |
16117.020 | 0.005 | 6204.6210 | 0.0020 | 6202.9561 | a3G4 | d3F2 | 14556 | 30673 | 9.10 × 10−2 | E2 |
16180.019 | 0.004 | 6180.4625 | 0.0014 | 6178.8039 | a3G3 | d3F3 | 14462 | 30642 | 8.90 × 10−2 | M1, E2 |
16211.340 | 0.005 | 6168.5215 | 0.0020 | 6166.8661 | a3G3 | d3F2 | 14462 | 30673 | 3.78 × 10−1 | M1, E2 |
16317.939 | 0.003 | 6128.2249 | 0.0011 | 6126.5799 | a1G4 | b1F3 | 17911 | 34229 | 4.78 × 10−2 | M1, E2 |
16348.985 | 0.003 | 6116.5877 | 0.0012 | 6114.9457 | a3F3 | b1D2 | 8842 | 25191 | 3.09 × 10−2 | M1, E2 |
16550.673 | 0.004 | 6042.0504 | 0.0013 | 6040.4278 | a3F2 | b1D2 | 8640 | 25191 | 1.53 × 10−2 | M1, E2 |
16697.450 | 0.003 | 5988.9384 | 0.0011 | 5987.3297 | b3F4 | c3F3 | 13609 | 30306 | 6.95 × 10−2 | M1, E2 |
16709.589 | 0.003 | 5984.5877 | 0.0011 | 5982.9800 | b3F4 | c3F4 | 13609 | 30319 | 2.45 × 10−1 | M1, E2 |
16724.866 | 0.005 | 5979.1211 | 0.0018 | 5977.5149 | b3F3 | c3F2 | 13543 | 30268 | 1.02 × 10−1 | M1, E2 |
16763.744 | 0.003 | 5965.2545 | 0.0011 | 5963.6519 | b3F3 | c3F3 | 13543 | 30306 | 1.81 × 10−1 | M1, E2 |
16775.883 | 0.003 | 5960.9381 | 0.0011 | 5959.3366 | b3F3 | c3F4 | 13543 | 30319 | 5.58 × 10−2 | M1, E2 |
16776.628 | 0.005 | 5960.6734 | 0.0019 | 5959.0720 | b3F2 | c3F2 | 13491 | 30268 | 2.33 × 10−1 | M1, E2 |
16815.506 | 0.004 | 5946.8921 | 0.0013 | 5945.2943 | b3F2 | c3F3 | 13491 | 30306 | 7.35 × 10−2 | M1, E2 |
17004.971 | 0.003 | 5880.6334 | 0.0011 | 5879.0528 | b3F4 | d3F4 | 13609 | 30614 | 5.13 × 10−2 | M1, E2 |
17032.828 | 0.003 | 5871.0157 | 0.0011 | 5869.4376 | b3F4 | d3F3 | 13609 | 30642 | 2.84 × 10−2 | M1, E2 |
17071.265 | 0.003 | 5857.7967 | 0.0011 | 5856.2220 | b3F3 | d3F4 | 13543 | 30614 | 1.31 × 10−2 | M1, E2 |
17099.122 | 0.003 | 5848.2535 | 0.0011 | 5846.6813 | b3F3 | d3F3 | 13543 | 30642 | 1.62 × 10−2 | M1, E2 |
17130.443 | 0.005 | 5837.5607 | 0.0017 | 5835.9912 | b3F3 | d3F2 | 13543 | 30673 | 2.31 × 10−2 | M1, E2 |
17182.205 | 0.005 | 5819.9748 | 0.0018 | 5818.4099 | b3F2 | d3F2 | 13491 | 30673 | 1.45 × 10−2 | M1, E2 |
17654.594 | 0.003 | 5664.2481 | 0.0010 | 5662.7236 | a5F4 | b3D3 | 2968 | 20623 | 4.21 × 10−2 | M1, E2 |
17722.411 | 0.005 | 5642.5731 | 0.0017 | 5641.0543 | a3H4 | c3F2 | 12545 | 30268 | 3.11 × 10−2 | E2 |
17808.114 | 0.003 | 5615.4178 | 0.0010 | 5613.9060 | a5F3 | b3D2 | 2809 | 20617 | 3.25 × 10−2 | M1, E2 |
17834.939 | 0.004 | 5606.9718 | 0.0013 | 5605.4622 | a5F2 | b3D1 | 2687 | 20522 | 4.50 × 10−2 | M1, E2 |
17907.832 | 0.003 | 5584.1489 | 0.0010 | 5582.6452 | a3H6 | d3F4 | 12706 | 30614 | 1.18 | E2 |
17917.107 | 0.004 | 5581.2582 | 0.0013 | 5579.7552 | a5F1 | b3D1 | 2605 | 20522 | 2.26 × 10−2 | M1, E2 |
17992.425 | 0.003 | 5557.8945 | 0.0010 | 5556.3976 | a3H5 | d3F4 | 12621 | 30614 | 1.27 × 10−1 | M1, E2 |
18020.282 | 0.003 | 5549.3027 | 0.0010 | 5547.8081 | a3H5 | d3F3 | 12621 | 30642 | 1.15 | E2 |
18096.667 | 0.004 | 5525.8794 | 0.0011 | 5524.3909 | a3H4 | d3F3 | 12545 | 30642 | 1.58 × 10−1 | M1, E2 |
18127.988 | 0.005 | 5516.3320 | 0.0016 | 5514.8459 | a3H4 | d3F2 | 12545 | 30673 | 1.29 | E2 |
18171.968 | 0.003 | 5502.9813 | 0.0010 | 5501.4986 | a5F3 | a1D2 | 2809 | 20981 | 1.71 × 10−2 | M1, E2 |
18398.128 | 0.004 | 5435.3356 | 0.0011 | 5433.8705 | a3P2 | c3F3 | 11908 | 30306 | 3.39 × 10−2 | M1, E2 |
18410.267 | 0.004 | 5431.7518 | 0.0011 | 5430.2875 | a3P2 | c3F4 | 11908 | 30319 | 9.30 × 10−2 | E2 |
18431.696 | 0.005 | 5425.4367 | 0.0015 | 5423.9741 | b3F4 | d3P2 | 13609 | 32041 | 1.06 × 10−1 | E2 |
18497.990 | 0.005 | 5405.9928 | 0.0015 | 5404.5352 | b3F3 | d3P2 | 13543 | 32041 | 2.72 × 10−2 | M1, E2 |
18752.727 | 0.005 | 5332.5578 | 0.0015 | 5331.1192 | a3P1 | c3F2 | 11515 | 30268 | 5.14 × 10−2 | M1, E2 |
18756.612 | 0.006 | 5331.4532 | 0.0017 | 5330.0150 | b3F3 | d3P1 | 13543 | 32299 | 1.01 × 10−1 | E2 |
18791.605 | 0.004 | 5321.5252 | 0.0010 | 5320.0895 | a3P1 | c3F3 | 11515 | 30306 | 6.96 × 10−2 | E2 |
18808.374 | 0.006 | 5316.7807 | 0.0018 | 5315.3462 | b3F2 | d3P1 | 13491 | 32299 | 5.01 × 10−2 | M1, E2 |
18929.167 | 0.010 | 5282.8526 | 0.0028 | 5281.4270 | b3F2 | d3P0 | 13491 | 32420 | 1.58 × 10−1 | E2 |
18971.998 | 0.007 | 5270.9261 | 0.0020 | 5269.5035 | a3P0 | c3F2 | 11296 | 30268 | 5.22 × 10−2 | E2 |
20132.374 | 0.005 | 4967.1241 | 0.0013 | 4965.7799 | a3P2 | d3P2 | 11908 | 32041 | 3.50 × 10−2 | M1, E2 |
20390.996 | 0.006 | 4904.1253 | 0.0015 | 4902.7974 | a3P2 | d3P1 | 11908 | 32299 | 7.02 × 10−2 | M1, E2 |
20511.789 | 0.010 | 4875.2452 | 0.0024 | 4873.9246 | a3P2 | d3P0 | 11908 | 32420 | 8.95 × 10−2 | E2 |
20525.851 | 0.005 | 4871.9052 | 0.0013 | 4870.5855 | a3P1 | d3P2 | 11515 | 32041 | 4.48 × 10−2 | M1, E2 |
20745.122 | 0.007 | 4820.4103 | 0.0016 | 4819.1039 | a3P0 | d3P2 | 11296 | 32041 | 1.99 × 10−2 | E2 |
20784.473 | 0.006 | 4811.2839 | 0.0015 | 4809.9798 | a3P1 | d3P1 | 11515 | 32299 | 2.30 × 10−2 | M1, E2 |
21208.500 | 0.003 | 4715.0906 | 0.0007 | 4713.8113 | a3F4 | c3F3 | 9098 | 30306 | 1.60 × 10−2 | M1, E2 |
21220.639 | 0.003 | 4712.3934 | 0.0007 | 4711.1148 | a3F4 | c3F4 | 9098 | 30319 | 4.26 × 10−2 | M1, E2 |
21425.461 | 0.005 | 4667.3441 | 0.0011 | 4666.0770 | a3F3 | c3F2 | 8842 | 30268 | 1.80 × 10−2 | M1, E2 |
21464.339 | 0.003 | 4658.8903 | 0.0007 | 4657.6253 | a3F3 | c3F3 | 8842 | 30306 | 2.73 × 10−2 | M1, E2 |
21516.021 | 0.003 | 4647.6995 | 0.0007 | 4646.4374 | a3F4 | d3F4 | 9098 | 30614 | 1.10 × 10−1 | M1, E2 |
21543.878 | 0.003 | 4641.6899 | 0.0007 | 4640.4293 | a3F4 | d3F3 | 9098 | 30642 | 2.89 × 10−2 | M1, E2 |
21627.149 | 0.005 | 4623.8180 | 0.0012 | 4622.5620 | a3F2 | c3F2 | 8640 | 30268 | 3.20 × 10−2 | M1, E2 |
21666.027 | 0.004 | 4615.5209 | 0.0008 | 4614.2671 | a3F2 | c3F3 | 8640 | 30306 | 1.07 × 10−2 | M1, E2 |
21771.860 | 0.003 | 4593.0848 | 0.0007 | 4591.8368 | a3F3 | d3F4 | 8842 | 30614 | 2.45 × 10−2 | M1, E2 |
21799.717 | 0.003 | 4587.2155 | 0.0007 | 4585.9690 | a3F3 | d3F3 | 8842 | 30642 | 8.08 × 10−2 | M1, E2 |
21831.038 | 0.005 | 4580.6342 | 0.0011 | 4579.3894 | a3F3 | d3F2 | 8842 | 30673 | 4.29 × 10−2 | M1, E2 |
22001.405 | 0.004 | 4545.1643 | 0.0007 | 4543.9285 | a3F2 | d3F3 | 8640 | 30642 | 3.16 × 10−2 | M1, E2 |
22032.726 | 0.005 | 4538.7030 | 0.0011 | 4537.4689 | a3F2 | d3F2 | 8640 | 30673 | 1.03 × 10−1 | M1, E2 |
32383.948 | 0.010 | 3087.9496 | 0.0010 | 3087.0801 | a5D1 | d3P0 | 36 | 32420 | 1.10 × 10−2 | M1 |
Notes. aCalculated using Birch & Downs (1994) for λvac > 7500 Å, and Bönsch & Potulski (1998) for all other cases. bTruncated energy. For the exact value, see Thorne et al. (2013). cCalculated transition probabilities derived from the log (gA) values given by Kurucz (2006b).
A machine-readable version of the table is available.
The structure of Co ii is only marginally less complex, with 47 metastable levels between the 3d8 a3D4 ground state and the 3d7(4F)4p z5F5 lowest-lying odd level at 45197.708(1) cm−1 (Pickering et al. 1998), as shown in Figure 2. Accurate energies for 41 of these levels are given by Pickering et al. (1998), and another five—the 3d64s2a5D1 level and the levels belonging to the c3F and a1F terms of the 3d7(2F)4s configuration—by Sugar & Corliss (1985). The final metastable level, 3d64s2a5D0, was omitted from our calculations as, to our knowledge, no experimental value exists for its energy.
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Standard image High-resolution imageBy again applying the selection rules in Table 1, we calculated accurate Ritz wavelengths for the 782 possible parity-forbidden [Co ii] lines originating from M1 and E2 transitions between the remaining 46 levels. The most significant lines are shown in Table 3, and the remaining weaker lines in Table 5. Where a transition takes place between levels reported by Pickering et al. (1998), the uncertainty in the Ritz wavenumber is as low as 0.001 cm−1, but for those that include the levels from Sugar & Corliss (1985), this value is an order of magnitude larger due to the lower accuracy with which those energy levels are known.
Table 3. Parity-forbidden Lines in Co ii with a Transition Probability of At Least 1 × 10−2 s−1 and Upper Level Excitation Less Than 5 eV
Wavenumber | Unc. | λvac | Unc. | λair | Transition | Energy (cm−1)b | A | Type | ||
---|---|---|---|---|---|---|---|---|---|---|
(cm−1) | (cm−1) | (Å) | (Å) | (Å)a | Lower | Upper | Lower | Upper | (s−1)c | |
Level | Level | Level | Level | |||||||
531.801 | 0.001 | 188040.2500 | 0.5001 | 187988.9985 | a5F4 | a5F3 | 4029 | 4561 | 1.09 × 10−2 | M1 |
678.494 | 0.001 | 147385.2282 | 0.3072 | 147345.0570 | a5F5 | a5F4 | 3350 | 4029 | 1.24 × 10−2 | M1 |
895.471 | 0.001 | 111673.0670 | 0.1764 | 111642.6289 | b3F4 | b3F3 | 9813 | 10708 | 1.88 × 10−2 | M1 |
950.324 | 0.002 | 105227.2625 | 0.2476 | 105198.5811 | a3F4 | a3F3 | 0 | 950 | 2.24 × 10−2 | M1 |
1156.905 | 0.003 | 86437.5147 | 0.2113 | 86413.9543 | a3D2 | a3D1 | 28112 | 29269 | 3.17 × 10−2 | M1 |
1243.097 | 0.001 | 80444.2397 | 0.0915 | 80422.3125 | b3P2 | c3P1 | 24074 | 25318 | 2.65 × 10−2 | M1 |
1609.411 | 0.002 | 62134.5281 | 0.0863 | 62117.5908 | a1D2 | a3P2 | 11651 | 13261 | 3.08 × 10−2 | M1 |
1683.639 | 0.002 | 59395.1512 | 0.0789 | 59378.9604 | a1P1 | a3D1 | 27585 | 29269 | 1.49 × 10−2 | M1 |
1753.044 | 0.001 | 57043.6298 | 0.0460 | 57028.0798 | a1D2 | a3P1 | 11651 | 13404 | 2.87 × 10−2 | M1 |
2267.621 | 0.001 | 44099.0770 | 0.0275 | 44087.0542 | c3P1 | a1P1 | 25318 | 27585 | 1.18 × 10−2 | M1 |
2321.755 | 0.001 | 43070.8636 | 0.0262 | 43059.1210 | b1G4 | a3H5 | 25147 | 27469 | 1.49 × 10−2 | M1 |
2597.973 | 0.002 | 38491.5444 | 0.0331 | 38481.0495 | c3P2 | a3D3 | 24886 | 27484 | 1.18 × 10−2 | M1 |
2754.928 | 0.002 | 36298.5868 | 0.0295 | 36288.6893 | b1G4 | a3H4 | 25147 | 27902 | 1.72 × 10−2 | M1 |
3173.659 | 0.001 | 31509.3692 | 0.0140 | 31500.7764 | b3P0 | a1P1 | 24411 | 27585 | 3.94 × 10−2 | M1 |
3225.472 | 0.002 | 31003.2122 | 0.0215 | 30994.7573 | c3P2 | a3D2 | 24886 | 28112 | 1.68 × 10−2 | M1 |
3317.756 | 0.001 | 30140.8521 | 0.0128 | 30132.6321 | b3P1 | a1P1 | 24267 | 27585 | 4.23 × 10−2 | M1 |
3407.455 | 0.003 | 29347.4141 | 0.0244 | 29339.4102 | c3P0 | a3D1 | 25861 | 29269 | 1.89 × 10−2 | M1 |
3409.953 | 0.002 | 29325.9153 | 0.0192 | 29317.9173 | b3P2 | a3D3 | 24074 | 27484 | 1.31 × 10−2 | M1 |
3461.429 | 0.002 | 28889.8004 | 0.0187 | 28881.9212 | a3H6 | a1H5 | 27106 | 30567 | 1.11 × 10−2 | M1 |
3510.718 | 0.001 | 28484.1998 | 0.0115 | 28476.4310 | b3P2 | a1P1 | 24074 | 27585 | 2.87 × 10−2 | M1 |
3522.704 | 0.001 | 28387.2823 | 0.0114 | 28379.5399 | a3G5 | b1G4 | 21625 | 25147 | 1.41 × 10−2 | M1 |
3614.274 | 0.002 | 27668.0719 | 0.0171 | 27660.5254 | a1P1 | b1D2 | 27585 | 31199 | 1.97 × 10−2 | M1 |
3715.039 | 0.003 | 26917.6159 | 0.0205 | 26910.2738 | a3D3 | b1D2 | 27484 | 31199 | 3.20 × 10−2 | M1 |
3951.260 | 0.002 | 25308.3809 | 0.0143 | 25301.4770 | c3P1 | a3D1 | 25318 | 29269 | 7.19 × 10−2 | M1 |
4037.452 | 0.002 | 24768.0946 | 0.0137 | 24761.3378 | b3P2 | a3D2 | 24074 | 28112 | 2.20 × 10−2 | M1 |
4382.377 | 0.002 | 22818.6651 | 0.0116 | 22812.4391 | c3P2 | a3D1 | 24886 | 29269 | 6.44 × 10−2 | M1 |
4857.298 | 0.002 | 20587.5763 | 0.0095 | 20581.9576 | b3P0 | a3D1 | 24411 | 29269 | 1.52 × 10−2 | M1 |
5481.215 | 0.002 | 18244.1289 | 0.0074 | 18239.1480 | a3G5 | a3H6 | 21625 | 27106 | 3.80 × 10−2 | M1 |
5487.730 | 0.002 | 18222.4696 | 0.0074 | 18217.4946 | a3G3 | a3H4 | 22414 | 27902 | 2.85 × 10−2 | M1 |
5844.459 | 0.001 | 17110.2223 | 0.0041 | 17105.5500 | a3G5 | a3H5 | 21625 | 27469 | 3.87 × 10−2 | M1 |
5892.816 | 0.002 | 16969.8143 | 0.0064 | 16965.1801 | a3G4 | a3H4 | 22009 | 27902 | 6.87 × 10−2 | M1 |
5928.741 | 0.002 | 16866.9863 | 0.0064 | 16862.3800 | a5P1 | b3P1 | 18339 | 24267 | 4.20 × 10−2 | M1 |
6072.838 | 0.002 | 16466.7645 | 0.0061 | 16462.2671 | a5P1 | b3P0 | 18339 | 24411 | 6.94 × 10−2 | M1 |
6117.161 | 0.001 | 16347.4515 | 0.0038 | 16342.9866 | a5F1 | b3F2 | 5205 | 11322 | 1.35 × 10−2 | M1 |
6302.912 | 0.001 | 15865.6813 | 0.0036 | 15861.3474 | a5P3 | b3P2 | 17772 | 24074 | 1.61 × 10−2 | M1 |
6313.012 | 0.002 | 15840.2983 | 0.0056 | 15835.9713 | c3P2 | b1D2 | 24886 | 31199 | 1.61 × 10−1 | M1 |
6462.365 | 0.001 | 15474.2100 | 0.0034 | 15469.9825 | a5F5 | b3F4 | 3350 | 9813 | 2.81 × 10−2 | M1 |
6547.759 | 0.002 | 15272.3998 | 0.0052 | 15268.2272 | a5P1 | c3P2 | 18339 | 24886 | 1.87 × 10−2 | M1 |
6854.972 | 0.001 | 14587.9506 | 0.0030 | 14583.9641 | a5P2 | c3P2 | 18031 | 24886 | 9.26 × 10−2 | M1 |
6932.030 | 0.002 | 14425.7877 | 0.0047 | 14421.8453 | b3P1 | b1D2 | 24267 | 31199 | 2.56 × 10−2 | M1 |
6978.876 | 0.002 | 14328.9540 | 0.0046 | 14325.0379 | a5P1 | c3P1 | 18339 | 25318 | 1.33 × 10−1 | M1 |
7114.892 | 0.001 | 14055.0261 | 0.0028 | 14051.1845 | a5P3 | c3P2 | 17772 | 24886 | 1.68 × 10−1 | M1 |
7522.682 | 0.003 | 13293.1322 | 0.0050 | 13289.4976 | a5P1 | c3P0 | 18339 | 25861 | 1.35 × 10−1 | M1 |
8557.829 | 0.001 | 11685.2072 | 0.0019 | 11682.0092 | a3G4 | a1H5 | 22009 | 30567 | 4.33 × 10−2 | M1 |
8942.645 | 0.001 | 11182.3744 | 0.0018 | 11179.3128 | a3G5 | a1H5 | 21625 | 30567 | 1.05 × 10−1 | M1 |
9246.498 | 0.002 | 10814.9057 | 0.0026 | 10811.9438 | a5P1 | a1P1 | 18339 | 27585 | 2.04 × 10−2 | M1 |
9452.946 | 0.002 | 10578.7131 | 0.0025 | 10575.8153 | a5P2 | a3D3 | 18031 | 27484 | 1.65 × 10−2 | M1 |
9712.866 | 0.002 | 10295.6227 | 0.0024 | 10292.8016 | a5P3 | a3D3 | 17772 | 27484 | 5.69 × 10−2 | M1 |
9724.663 | 0.002 | 10283.1330 | 0.0024 | 10280.3153 | a3F2 | b3F2 | 1597 | 11322 | 2.69 × 10−2 | M1, E2 |
9758.007 | 0.002 | 10247.9946 | 0.0023 | 10245.1865 | a3F3 | b3F3 | 950 | 10708 | 2.25 × 10−2 | E2 |
9773.232 | 0.003 | 10232.0300 | 0.0030 | 10229.2262 | a5P1 | a3D2 | 18339 | 28112 | 1.21 × 10−2 | M1 |
9812.860 | 0.001 | 10190.7093 | 0.0015 | 10187.9166 | a3F4 | b3F4 | 0 | 9813 | 3.43 × 10−2 | E2 |
10054.080 | 0.002 | 9946.2112 | 0.0022 | 9943.4848 | a3F2 | a1D2 | 1597 | 11651 | 7.91 × 10−2 | M1, E2 |
10080.445 | 0.002 | 9920.1973 | 0.0022 | 9917.4779 | a5P2 | a3D2 | 18031 | 28112 | 4.37 × 10−2 | M1 |
10371.536 | 0.002 | 9641.7737 | 0.0021 | 9639.1298 | a3F3 | b3F2 | 950 | 11322 | 2.02 × 10−2 | M1, E2 |
10700.953 | 0.002 | 9344.9623 | 0.0020 | 9342.3988 | a3F3 | a1D2 | 950 | 11651 | 1.71 × 10−1 | M1 |
10708.331 | 0.001 | 9338.5237 | 0.0012 | 9335.9619 | a3F4 | b3F3 | 0 | 10708 | 1.51 × 10−2 | E2 |
10863.061 | 0.001 | 9205.5087 | 0.0012 | 9202.9829 | a3P1 | b3P1 | 13404 | 24267 | 1.18 × 10−2 | E2 |
11006.694 | 0.002 | 9085.3804 | 0.0018 | 9082.8872 | a3P2 | b3P1 | 13261 | 24267 | 2.33 × 10−2 | E2 |
11092.571 | 0.001 | 9015.0428 | 0.0011 | 9012.5686 | b3F2 | a3G3 | 11322 | 22414 | 2.39 × 10−2 | M1 |
11150.791 | 0.002 | 8967.9738 | 0.0018 | 8965.5124 | a3P2 | b3P0 | 13261 | 24411 | 4.62 × 10−2 | E2 |
11482.079 | 0.001 | 8709.2243 | 0.0011 | 8706.8328 | a3P1 | c3P2 | 13404 | 24886 | 1.88 × 10−2 | E2 |
11593.446 | 0.001 | 8625.5632 | 0.0011 | 8623.1944 | a1G4 | a1H5 | 18974 | 30567 | 8.28 × 10−2 | E2 |
11625.712 | 0.002 | 8601.6238 | 0.0017 | 8599.2615 | a3P2 | c3P2 | 13261 | 24886 | 1.18 × 10−2 | E2 |
11663.491 | 0.003 | 8573.7625 | 0.0021 | 8571.4076 | a3F2 | a3P2 | 1597 | 13261 | 1.75 × 10−2 | M1 |
11706.100 | 0.001 | 8542.5549 | 0.0010 | 8540.2085 | b3F3 | a3G3 | 10708 | 22414 | 3.93 × 10−2 | M1 |
11811.669 | 0.001 | 8466.2042 | 0.0010 | 8463.8784 | b3F4 | a3G5 | 9813 | 21625 | 3.78 × 10−2 | M1 |
11996.091 | 0.004 | 8336.0489 | 0.0025 | 8333.7583 | a3F2 | a3P0 | 1597 | 13593 | 3.11 × 10−2 | E2 |
12196.485 | 0.001 | 8199.0837 | 0.0010 | 8196.8301 | b3F4 | a3G4 | 9813 | 22009 | 4.85 × 10−2 | M1 |
12310.364 | 0.003 | 8123.2367 | 0.0019 | 8121.0037 | a3F3 | a3P2 | 950 | 13261 | 6.77 × 10−2 | M1, E2 |
12453.997 | 0.002 | 8029.5508 | 0.0014 | 8027.3430 | a3F3 | a3P1 | 950 | 13404 | 2.45 × 10−2 | E2 |
12616.105 | 0.001 | 7926.3767 | 0.0009 | 7924.1968 | a1D2 | b3P1 | 11651 | 24267 | 4.20 × 10−2 | E2 |
12760.202 | 0.001 | 7836.8666 | 0.0009 | 7834.7108 | a1D2 | b3P0 | 11651 | 24411 | 4.12 × 10−2 | E2 |
12945.522 | 0.001 | 7724.6789 | 0.0008 | 7722.5534 | b3F2 | b3P1 | 11322 | 24267 | 1.52 × 10−2 | E2 |
13089.619 | 0.001 | 7639.6418 | 0.0008 | 7637.5393 | b3F2 | b3P0 | 11322 | 24411 | 2.12 × 10−2 | E2 |
13133.942 | 0.002 | 7613.8604 | 0.0013 | 7611.7648 | a5F1 | a5P1 | 5205 | 18339 | 1.23 × 10−2 | E2 |
13235.123 | 0.001 | 7555.6533 | 0.0008 | 7553.5734 | a1D2 | c3P2 | 11651 | 24886 | 1.90 × 10−2 | M1, E2 |
13260.688 | 0.002 | 7541.0869 | 0.0013 | 7539.0110 | a3F4 | a3P2 | 0 | 13261 | 2.80 × 10−2 | E2 |
13388.578 | 0.002 | 7469.0531 | 0.0012 | 7467.0583 | a5F2 | a5P1 | 4950 | 18339 | 1.50 × 10−2 | E2 |
13470.638 | 0.001 | 7423.5534 | 0.0008 | 7421.5705 | a5F3 | a5P2 | 4561 | 18031 | 1.39 × 10−2 | E2 |
13495.956 | 0.001 | 7409.6270 | 0.0008 | 7407.6477 | a1D2 | b1G4 | 11651 | 25147 | 5.39 × 10−2 | E2 |
13559.051 | 0.001 | 7375.1474 | 0.0008 | 7373.1772 | b3F3 | b3P1 | 10708 | 24267 | 2.35 × 10−2 | E2 |
13564.540 | 0.001 | 7372.1630 | 0.0008 | 7370.1935 | b3F2 | c3P2 | 11322 | 24886 | 1.81 × 10−2 | M1 |
13742.519 | 0.001 | 7276.6863 | 0.0007 | 7274.7418 | a5F4 | a5P3 | 4029 | 17772 | 1.05 × 10−2 | E2 |
13777.851 | 0.002 | 7258.0260 | 0.0012 | 7256.0863 | a5F3 | a5P1 | 4561 | 18339 | 1.04 × 10−2 | E2 |
14002.439 | 0.001 | 7141.6130 | 0.0007 | 7139.7037 | a5F4 | a5P2 | 4029 | 18031 | 2.00 × 10−2 | E2 |
14178.069 | 0.001 | 7053.1467 | 0.0007 | 7051.2605 | b3F3 | c3P2 | 10708 | 24886 | 1.03 × 10−2 | M1, E2 |
14180.817 | 0.001 | 7051.7799 | 0.0007 | 7049.8941 | a3P1 | a1P1 | 13404 | 27585 | 2.02 × 10−2 | M1, E2 |
14223.685 | 0.003 | 7030.5269 | 0.0014 | 7028.6467 | a3P2 | a3D3 | 13261 | 27484 | 1.07 × 10−2 | M1, E2 |
14261.560 | 0.001 | 7011.8556 | 0.0007 | 7009.9803 | b3F4 | b3P2 | 9813 | 24074 | 2.61 × 10−2 | E2 |
14324.450 | 0.002 | 6981.0708 | 0.0011 | 6979.2035 | a3P2 | a1P1 | 13261 | 27585 | 4.70 × 10−2 | E2 |
14421.013 | 0.001 | 6934.3256 | 0.0007 | 6932.4705 | a5F5 | a5P3 | 3350 | 17772 | 3.68 × 10−2 | E2 |
14438.902 | 0.001 | 6925.7344 | 0.0007 | 6923.8815 | b3F3 | b1G4 | 10708 | 25147 | 1.11 × 10−1 | M1 |
14851.184 | 0.003 | 6733.4699 | 0.0013 | 6731.6672 | a3P2 | a3D2 | 13261 | 28112 | 1.53 × 10−2 | E2 |
15073.540 | 0.001 | 6634.1417 | 0.0006 | 6632.3649 | b3F4 | c3P2 | 9813 | 24886 | 1.65 × 10−2 | E2 |
15334.373 | 0.001 | 6521.2969 | 0.0006 | 6519.5496 | b3F4 | b1G4 | 9813 | 25147 | 1.93 × 10−1 | M1 |
15933.861 | 0.001 | 6275.9427 | 0.0006 | 6274.2593 | a1D2 | a1P1 | 11651 | 27585 | 1.31 × 10−1 | E2 |
16008.089 | 0.003 | 6246.8418 | 0.0011 | 6245.1659 | a3P2 | a3D1 | 13261 | 29269 | 1.16 × 10−1 | E2 |
16250.884 | 0.002 | 6153.5114 | 0.0008 | 6151.8598 | a1D2 | a3H4 | 11651 | 27902 | 1.14 × 10−2 | E2 |
16263.278 | 0.001 | 6148.8219 | 0.0005 | 6147.1715 | b3F2 | a1P1 | 11322 | 27585 | 2.52 × 10−2 | M1 |
16776.042 | 0.002 | 5960.8815 | 0.0008 | 5959.2801 | b3F3 | a3D3 | 10708 | 27484 | 6.83 × 10−2 | M1 |
16790.012 | 0.002 | 5955.9218 | 0.0008 | 5954.3217 | b3F2 | a3D2 | 11322 | 28112 | 3.42 × 10−2 | M1 |
17376.530 | 0.002 | 5754.8889 | 0.0007 | 5753.3409 | a3F2 | a1G4 | 1597 | 18974 | 3.76 × 10−2* | E2 |
17403.541 | 0.002 | 5745.9570 | 0.0007 | 5744.4114 | b3F3 | a3D2 | 10708 | 28112 | 1.34 × 10−2 | M1 |
17448.555 | 0.001 | 5731.1335 | 0.0005 | 5729.5917 | a5F3 | a3G4 | 4561 | 22009 | 9.63 × 10−2 | M1 |
17464.368 | 0.001 | 5725.9443 | 0.0005 | 5724.4039 | a5F2 | a3G3 | 4950 | 22414 | 6.65 × 10−2 | M1 |
17595.540 | 0.001 | 5683.2583 | 0.0005 | 5681.7289 | a5F4 | a3G5 | 4029 | 21625 | 7.93 × 10−2 | M1 |
17617.500 | 0.002 | 5676.1742 | 0.0007 | 5674.6466 | a1D2 | a3D1 | 11651 | 29269 | 1.96 × 10−1 | E2 |
17671.513 | 0.002 | 5658.8249 | 0.0007 | 5657.3019 | b3F4 | a3D3 | 9813 | 27484 | 1.19 × 10−1 | M1 |
17853.641 | 0.001 | 5601.0983 | 0.0004 | 5599.5902 | a5F3 | a3G3 | 4561 | 22414 | 8.70 × 10−2 | M1 |
17938.724 | 0.003 | 5574.5324 | 0.0009 | 5573.0312 | a3P2 | b1D2 | 13261 | 31199 | 1.63 × 10−1 | E2 |
17946.917 | 0.002 | 5571.9876 | 0.0007 | 5570.4870 | b3F2 | a3D1 | 11322 | 29269 | 4.76 × 10−2 | M1, E2 |
17980.356 | 0.001 | 5561.6251 | 0.0004 | 5560.1272 | a5F4 | a3G4 | 4029 | 22009 | 2.20 × 10−1 | M1 |
18023.403 | 0.002 | 5548.3417 | 0.0007 | 5546.8473 | a3F3 | a1G4 | 950 | 18974 | 7.09 × 10−2 | M1 |
18274.034 | 0.001 | 5472.2454 | 0.0004 | 5470.7707 | a5F5 | a3G5 | 3350 | 21625 | 3.92 × 10−1 | M1 |
18385.442 | 0.001 | 5439.0859 | 0.0004 | 5437.6198 | a5F4 | a3G3 | 4029 | 22414 | 1.45 × 10−2 | M1 |
18658.850 | 0.001 | 5359.3870 | 0.0004 | 5357.9415 | a5F5 | a3G4 | 3350 | 22009 | 2.33 × 10−2 | M1 |
18973.727 | 0.001 | 5270.4457 | 0.0004 | 5269.0232 | a3F4 | a1G4 | 0 | 18974 | 1.38 × 10−1 | M1 |
19513.630 | 0.001 | 5124.6231 | 0.0004 | 5123.2382 | a5F3 | b3P2 | 4561 | 24074 | 1.69 × 10−2 | M1 |
19548.135 | 0.002 | 5115.5774 | 0.0006 | 5114.1949 | a1D2 | b1D2 | 11651 | 31199 | 7.10 × 10−1 | M1, E2 |
19877.552 | 0.002 | 5030.8005 | 0.0006 | 5029.4399 | b3F2 | b1D2 | 11322 | 31199 | 3.23 × 10−1 | M1, E2 |
20112.818 | 0.001 | 4971.9536 | 0.0003 | 4970.6082 | a5F1 | c3P1 | 5205 | 25318 | 2.28 × 10−2 | M1 |
20325.610 | 0.001 | 4919.9014 | 0.0003 | 4918.5694 | a5F3 | c3P2 | 4561 | 24886 | 3.03 × 10−2 | M1 |
20367.454 | 0.001 | 4909.7937 | 0.0003 | 4908.4643 | a5F2 | c3P1 | 4950 | 25318 | 2.81 × 10−2 | M1 |
20412.147 | 0.002 | 4899.0436 | 0.0005 | 4897.7169 | a3F2 | a3G4 | 1597 | 22009 | 2.84 × 10−2 | E2 |
20491.081 | 0.002 | 4880.1719 | 0.0005 | 4878.8501 | b3F3 | b1D2 | 10708 | 31199 | 5.83 × 10−1 | M1 |
20674.204 | 0.002 | 4836.9455 | 0.0005 | 4835.6348 | a3F3 | a3G5 | 950 | 21625 | 2.56 × 10−2 | E2 |
20817.233 | 0.002 | 4803.7123 | 0.0005 | 4802.4101 | a3F2 | a3G3 | 1597 | 22414 | 4.41 × 10−1 | E2 |
21059.020 | 0.002 | 4748.5589 | 0.0005 | 4747.2710 | a3F3 | a3G4 | 950 | 22009 | 4.64 × 10−1 | E2 |
21464.107 | 0.002 | 4658.9407 | 0.0005 | 4657.6758 | a3F3 | a3G3 | 950 | 22414 | 1.26 × 10−1 | E2 |
21624.529 | 0.001 | 4624.3783 | 0.0003 | 4623.1222 | a3F4 | a3G5 | 0 | 21625 | 6.38 × 10−1 | E2 |
22009.345 | 0.001 | 4543.5247 | 0.0003 | 4542.2893 | a3F4 | a3G4 | 0 | 22009 | 1.03 × 10−1 | E2 |
22380.440 | 0.001 | 4468.1875 | 0.0003 | 4466.9714 | a5F1 | a1P1 | 5205 | 27585 | 1.61 × 10−1 | M1 |
22477.223 | 0.002 | 4448.9482 | 0.0004 | 4447.7371 | a3F2 | b3P2 | 1597 | 24074 | 2.96 × 10−2 | E2 |
22534.311 | 0.002 | 4437.6774 | 0.0004 | 4436.4691 | a5F2 | a3D3 | 4950 | 27484 | 2.91 × 10−2 | M1 |
22635.076 | 0.001 | 4417.9221 | 0.0003 | 4416.7189 | a5F2 | a1P1 | 4950 | 27585 | 3.48 × 10−1 | M1 |
22670.185 | 0.002 | 4411.0801 | 0.0004 | 4409.8786 | a3F2 | b3P1 | 1597 | 24267 | 3.19 × 10−1 | E2 |
22814.282 | 0.002 | 4383.2193 | 0.0004 | 4382.0250 | a3F2 | b3P0 | 1597 | 24411 | 4.14 × 10−1 | E2 |
22907.174 | 0.002 | 4365.4447 | 0.0004 | 4364.2549 | a5F1 | a3D2 | 5205 | 28112 | 7.17 × 10−2 | M1 |
22923.584 | 0.002 | 4362.3197 | 0.0004 | 4361.1307 | a5F3 | a3D3 | 4561 | 27484 | 1.31 × 10−2 | M1 |
23124.096 | 0.002 | 4324.4934 | 0.0004 | 4323.3141 | a3F3 | b3P2 | 950 | 24074 | 3.58 × 10−1 | E2 |
23161.810 | 0.002 | 4317.4519 | 0.0004 | 4316.2744 | a5F2 | a3D2 | 4950 | 28112 | 6.63 × 10−2 | M1 |
23317.058 | 0.002 | 4288.7058 | 0.0004 | 4287.5356 | a3F3 | b3P1 | 950 | 24267 | 4.65 × 10−1 | E2 |
23455.385 | 0.002 | 4263.4133 | 0.0004 | 4262.2496 | a5F4 | a3D3 | 4029 | 27484 | 5.91 × 10−1 | M1 |
23550.036 | 0.002 | 4246.2781 | 0.0004 | 4245.1187 | a3F2 | b1G4 | 1597 | 25147 | 9.41 × 10−2 | E2 |
23551.083 | 0.002 | 4246.0893 | 0.0004 | 4244.9299 | a5F3 | a3D2 | 4561 | 28112 | 7.62 × 10−1 | M1 |
23720.320 | 0.002 | 4215.7948 | 0.0004 | 4214.6432 | a3F2 | c3P1 | 1597 | 25318 | 3.75 × 10−1 | E2 |
24064.079 | 0.002 | 4155.5715 | 0.0004 | 4154.4352 | a5F1 | a3D1 | 5205 | 29269 | 1.74 × 10−1 | M1 |
24074.420 | 0.001 | 4153.7865 | 0.0002 | 4152.6507 | a3F4 | b3P2 | 0 | 24074 | 2.41 | E2 |
24264.125 | 0.003 | 4121.3108 | 0.0005 | 4120.1832 | a3F2 | c3P0 | 1597 | 25861 | 2.46 | E2 |
24318.715 | 0.002 | 4112.0594 | 0.0004 | 4110.9342 | a5F2 | a3D1 | 4950 | 29269 | 3.71 × 10−1 | M1 |
24367.193 | 0.002 | 4103.8786 | 0.0004 | 4102.7554 | a3F3 | c3P1 | 950 | 25318 | 1.65 | E2 |
24886.400 | 0.001 | 4018.2590 | 0.0002 | 4017.1576 | a3F4 | c3P2 | 0 | 24886 | 3.88 × 10−2 | E2 |
25147.233 | 0.001 | 3976.5807 | 0.0002 | 3975.4898 | a3F4 | b1G4 | 0 | 25147 | 1.29 × 10−2 | M1, E2 |
25887.176 | 0.003 | 3862.9166 | 0.0004 | 3861.8544 | a3F2 | a3D3 | 1597 | 27484 | 3.74 × 10−2 | E2 |
25987.941 | 0.002 | 3847.9386 | 0.0003 | 3846.8802 | a3F2 | a1P1 | 1597 | 27585 | 4.94 × 10−1 | E2 |
26304.964 | 0.003 | 3801.5639 | 0.0004 | 3800.5172 | a3F2 | a3H4 | 1597 | 27902 | 1.50 | E2 |
26514.675 | 0.003 | 3771.4964 | 0.0004 | 3770.4573 | a3F2 | a3D2 | 1597 | 28112 | 5.27 × 10−1 | E2 |
26518.664 | 0.002 | 3770.9291 | 0.0003 | 3769.8901 | a3F3 | a3H5 | 950 | 27469 | 1.73 | E2 |
26534.049 | 0.003 | 3768.7426 | 0.0004 | 3767.7042 | a3F3 | a3D3 | 950 | 27484 | 3.84 × 10−1 | E2 |
26634.814 | 0.002 | 3754.4847 | 0.0003 | 3753.4498 | a3F3 | a1P1 | 950 | 27585 | 2.71 × 10−1 | E2 |
26951.837 | 0.003 | 3710.3222 | 0.0004 | 3709.2985 | a3F3 | a3H4 | 950 | 27902 | 1.40 × 10−1 | E2 |
27105.744 | 0.002 | 3689.2550 | 0.0003 | 3688.2365 | a3F4 | a3H6 | 0 | 27106 | 2.06 | E2 |
27161.548 | 0.003 | 3681.6753 | 0.0004 | 3680.6588 | a3F3 | a3D2 | 950 | 28112 | 1.06 | E2 |
27468.988 | 0.001 | 3640.4690 | 0.0002 | 3639.4628 | a3F4 | a3H5 | 0 | 27469 | 1.05 × 10−1 | E2 |
27484.373 | 0.002 | 3638.4312 | 0.0003 | 3637.4255 | a3F4 | a3D3 | 0 | 27484 | 1.35 | E2 |
27671.580 | 0.003 | 3613.8161 | 0.0004 | 3612.8165 | a3F2 | a3D1 | 1597 | 29269 | 8.69 × 10−1 | E2 |
28111.872 | 0.002 | 3557.2160 | 0.0003 | 3556.2306 | a3F4 | a3D2 | 0 | 28112 | 9.09 × 10−2 | E2 |
28318.453 | 0.003 | 3531.2663 | 0.0004 | 3530.2874 | a3F3 | a3D1 | 950 | 29269 | 4.61 × 10−2 | E2 |
29616.849 | 0.002 | 3376.4564 | 0.0003 | 3375.5160 | a3F3 | a1H5 | 950 | 30567 | 4.39 × 10−2 | E2 |
30249.088 | 0.003 | 3305.8848 | 0.0003 | 3304.9618 | a3F3 | b1D2 | 950 | 31199 | 1.50 × 10−2 | M1, E2 |
Notes. aCalculated using Birch & Downs (1994) for λvac > 7500 Å, and Bönsch & Potulski (1998) for all other cases. bTruncated energy. For the exact value, scale the energies given in Pickering et al. (1998) by 7 parts in 108. cCalculated transition probabilities taken from Raassen et al. (1998). The line at 17376.531 cm−1 (*) is not given by Raassen et al. (1998), so the value shown is from Quinet (1998).
A machine-readable version of the table is available.
Table 4. Parity-forbidden Lines in V ii with a Transition Probability Less Than 1 × 10−2 s−1 or Upper Level Excitation Greater Than 5 eV
Wavenumber | Unc. | λvac | Unc. | λair | Transition | Energy (cm−1)b | A | Type | ||
---|---|---|---|---|---|---|---|---|---|---|
(cm−1) | (cm−1) | (Å) | (Å) | (Å)a | Lower | Upper | Lower | Upper | (s−1)c | |
Level | Level | Level | Level | |||||||
4.892 | 0.004 | 20441537.2036 | 17728.1475 | 20435965.8233 | b3P0 | b3P1 | 19161 | 19166 | 1.79 × 10−9 | M1 |
5.910 | 0.004 | 16920473.7733 | 12146.7835 | 16915862.0656 | b3D2 | b3D3 | 20617 | 20623 | 2.29 × 10−9 | M1, E2 |
12.139 | 0.004 | 8237910.8658 | 2879.1907 | 8235665.6073 | c3F3 | c3F4 | 30306 | 30319 | 3.62 × 10−8 | M1, E2 |
14.216 | 0.004 | 7034327.5183 | 2040.1854 | 7032410.2988 | a5P2 | b3F4 | 13595 | 13609 | 1.17 × 10−18 | E2 |
19.862 | 0.003 | 5034739.7040 | 801.5932 | 5033367.4759 | b1G4 | b3P2 | 19113 | 19133 | 3.80 × 10−19 | E2 |
20.916 | 0.003 | 4781028.8774 | 646.5286 | 4779725.7988 | b3F2 | a5P1 | 13491 | 13512 | 2.43 × 10−18 | E2 |
24.357 | 0.004 | 4105595.9272 | 607.7488 | 4104476.9391 | a3D1 | a3D2 | 18270 | 18294 | 3.14 × 10−7 | M1, E2 |
27.857 | 0.004 | 3589761.9988 | 546.7233 | 3588783.6022 | d3F4 | d3F3 | 30614 | 30642 | 5.57 × 10−7 | M1, E2 |
28.631 | 0.004 | 3492717.6836 | 517.5630 | 3491765.7367 | b3P2 | b3P0 | 19133 | 19161 | 5.03 × 10−16 | E2 |
30.846 | 0.002 | 3241911.4310 | 235.0105 | 3241027.8417 | a5P1 | b3F3 | 13512 | 13543 | 1.79 × 10−17 | E2 |
Notes. aCalculated using Birch & Downs (1994) for λvac > 7500 Å, and Bönsch & Potulski (1998) for all other cases. bTruncated energy. For the exact value, see Thorne et al. (2013). cCalculated transition probabilities derived from the log (gA) values given by Kurucz (2006b).
Only a portion of this table is shown here to demonstrate its form and content. A machine-readable version of the full table is available.
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Table 5. Parity-forbidden Lines in Co ii with a Transition Probability Less Than 1 × 10−2 s−1 or Upper Level Excitation Greater Than 5 eV
Wavenumber | Unc. | λvac | Unc. | λair | Transition | Energy (cm−1)b | A | Type | ||
---|---|---|---|---|---|---|---|---|---|---|
(cm−1) | (cm−1) | (Å) | (Å) | (Å)a | Lower | Upper | Lower | Upper | (s−1)c | |
Level | Level | Level | Level | |||||||
15.385 | 0.002 | 6499837.0491 | 944.6914 | 6498065.5060 | a3H5 | a3D3 | 27469 | 27484 | 2.03 × 10−20 | E2 |
76.085 | 0.031 | 1314319.4191 | 536.3402 | 1313961.1987 | a5D4 | c3F2 | 40695 | 40771 | ||
100.765 | 0.002 | 992408.0087 | 22.0224 | 992137.5259 | a3D3 | a1P1 | 27484 | 27585 | 4.86 × 10−17 | E2 |
108.330 | 0.042 | 923105.2617 | 361.5253 | 922853.6674 | c3F2 | c3F3 | 40771 | 40879 | 3.28 × 10−5 | M1, E2 |
143.633 | 0.002 | 696218.7868 | 10.8387 | 696029.0308 | a3P2 | a3P1 | 13261 | 13404 | 5.18 × 10−5 | M1, E2 |
144.097 | 0.001 | 693976.9253 | 6.8109 | 693787.7803 | b3P1 | b3P0 | 24267 | 24411 | 1.44 × 10−4 | M1 |
167.620 | 0.042 | 596587.4776 | 151.0026 | 596424.8763 | c3F3 | c3F4 | 40879 | 41047 | 9.50 × 10−5 | M1, E2 |
184.415 | 0.031 | 542255.2016 | 91.2948 | 542107.4086 | a5D4 | c3F3 | 40695 | 40879 | 4.78 × 10−9 | M1, E2 |
188.967 | 0.003 | 529192.8908 | 8.8558 | 529048.6580 | a3P1 | a3P0 | 13404 | 13593 | 3.64 × 10−4 | M1 |
192.962 | 0.001 | 518236.7150 | 3.7981 | 518095.4683 | b3P2 | b3P1 | 24074 | 24267 | 8.14 × 10−5 | M1, E2 |
Notes. aCalculated using Birch & Downs (1994) for λvac > 7500 Å, and Bönsch & Potulski (1998) for all other cases. bTruncated energy. For the exact value, scale the energies given in Pickering et al. (1998) by 7 parts in 108. cCalculated transition probabilities of 1 × 10−3 or greater were taken from Raassen et al. (1998) unless marked with a * or †. Values less than 1 × 10−3 were derived from the log (gA) values given by Kurucz (2006b). *Transition probability greater than 1 × 10−3 taken from Quinet (1998). †Transition probability greater than 1 × 10−3 derived from the log (gA) values given by Kurucz (2006b).
Only a portion of this table is shown here to demonstrate its form and content. A machine-readable version of the full table is available.
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3.2. Transition Probabilities
Also included in Tables 2–5 are calculated transition probabilities, A. In general, these were derived from the log (gA) values in Kurucz (2006a, 2006b), but for Co ii, the more detailed calculations reported by Raassen et al. (1998) and Quinet (1998) were used instead, where available.
The transition probabilities of Raassen et al. (1998) were obtained through a semi-empirical method. First, the angular coefficients of the transition matrix in pure LS coupling were found using the Racah algebra, multiplied by transition integrals from a relativistic Hartree–Fock code (Parpia et al. 1996), and corrected for core polarization (Hameed 1972; Laughlin 1992). The resulting LS transition matrix was then transformed into the actual intermediate coupling by using orthogonal operators (Hansen et al. 1998); adjusting the parameters of the model Hamiltonian to yield eigenvalues as close as possible to the experimental energies of Pickering et al. (1998).
Quinet (1998) used the approximately relativistic Hartree–Fock method (Cowan & Griffin 1976), followed by a least-squares optimization of the radial parameters to reduce discrepancies between calculated energy levels and the experimental levels reported by Sugar & Corliss (1985). Quinet (1998) also noted that strong multiplets are typically composed of only one type of transition; M1 transitions being dominant for inter-combination multiplets (ΔS ≠ 0) and E2 transitions dominating under LS-coupled selection rules (ΔS = 0).
A comparison of the transition probabilities obtained by Raassen et al. (1998), AR, with those obtained by Quinet (1998), AQ, is shown in Figure 3. Here, it can be seen that for the majority of lines, AR and AQ differ by no more than about 25%, although at values of AR less than 0.1 s−1, there is a significant minority of lines where differences increase to around a factor of two. At higher values of AR, the two sets of results converge, but rather than approaching zero difference, there is a systematic difference; AQ being approximately 25% larger than AR at values of AR greater than 0.1 s−1.
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Standard image High-resolution imageIn this paper, we choose to adopt the values given by Raassen et al. (1998), where possible, as these authors employed the more accurate and new energy levels of Pickering et al. (1998) in their calculations. We therefore only include values from Quinet (1998) in Tables 3 and 5 where no corresponding value is available in Raassen et al. (1998). If neither author reports a transition probability for a given line, as is the case for A < 1 × 10−3 s−1, the transition probability shown in Tables 3 and 5 is derived from the log (gA) values in Kurucz (2006b).
3.3. Air Wavelengths
In addition to the vacuum Ritz wavelengths for [V ii] and [Co ii] lines, Tables 2–5 also list the calculated air wavelength of each line, λair. Aldenius & Johansson (2007) give a detailed review of approaches to calculating λair in different spectral regions. Following their approach, the refractive index correction given by Birch & Downs (1994) was used for lines in the infrared (λvac > 7500 Å). For all lines of shorter wavelength, the correction given by Bönsch & Potulski (1998) was used.
4. SUMMARY
We have presented a comprehensive list of accurate Ritz wavelengths for parity-forbidden [Co ii] and [V ii] lines, calculated by considering radiative M1 and E2 transitions between all known metastable levels in each species. These data will aid the analysis of spectra from low-density astrophysical plasmas, particularly in the infrared where strong forbidden lines are seen in both the near-IR, from transitions between LS terms, and far-IR, from transitions between fine-structure levels.
We thank M. J. Barlow, P. J. Storey, and R. L. Kurucz for helpful discussions, and the UK Science and Technology Facilities Council (STFC) for funding this research.
Footnotes
- 1
Exceptions include levels that are metastable to E1, M1, and E2 transitions, such as the 1s22s2s3P2 level in Be-like ions. In this case, decay to the 1s22s2 1S0 involves ΔJ = 2 and occurs through a magnetic quadrupole (M2) transition.