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Power law statistics and stellar rotational velocities in the Pleiades

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Published 12 December 2008 Europhysics Letters Association
, , Citation J. C. Carvalho et al 2008 EPL 84 59001 DOI 10.1209/0295-5075/84/59001

0295-5075/84/5/59001

Abstract

In this paper we will show that, the non-Gaussian statistics framework based on the Kaniadakis statistics is more appropriate to fit the observed distributions of projected rotational velocity measurements of stars in the Pleiades open cluster. To this end, we compare the results from the κ and q-distributions with the Maxwellian.

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10.1209/0295-5075/84/59001