The spectral line shape model recently proposed by the present authors [J.
Chem. Phys. 109, 8283 (1998)] is extended in order to account for correlati
on between velocity- and phase-changing collisions. The possible additional
source of asymmetry due to the finite duration of collision is also includ
ed. In this implemented form, the model is consistent with previous exhaust
ive experimental studies in the collision regime for H-2-rare gases and H-2
-nitrogen mixtures and has been shown to also accurately describe the obser
ved spectral features at lower pressure for H-2-Ar. It should be pertinent
for various other molecular systems in a wide range of pressure and tempera
ture, in particular for optical diagnostics. (C) 1999 American Institute of
Physics. [S0021-9606(99)01927-3].