The relatively large probability of the fine-structure transitions (3P0-1, 3P0-2) which are observed in Ne*-Ne collisions at thermal energies (E>or=80 meV) cannot be accounted for by the spin-orbit (SO) interaction. The Ar2* system is in some ways similar to Ne2*, apart from a larger SO interaction. The probability of the 3P0 to 2 transition induced by the SO interaction is calculated for the Ar*-Ar collision at 326 meV. This probability is relatively weak ( approximately=2.6*10-2). The effect of the rotational coupling (L+or-) between Gamma states 3 Sigma g+ and 3 Pi g, which are degenerate at infinite R, is then examined in the framework of a simplified two-state (0g-, 1g) model. In Ar2, a larger transition probability ( approximately 0.1) is obtained for relatively large values of the angular momentum (l approximately=100-200). It seems however that this effect alone is not sufficient to explain the experimental data on Ne. In this latter case, an accidental degeneracy of 3 Sigma g+ and 3 Pi g potentials (shifted by the SO interaction) appears at finite distance ( approximately=6 au). It reinforces the effect of the rotational coupling and may give sufficiently large 3P0 to 1,2 transition probabilities at low energy and small l.