M. Contini et Sm. Viegas, SHOCK AND PHOTOIONIZATION MODELS FOR INFRARED LINES FROM ACTIVE GALACTIC NUCLEI, Astrophysics and space science, 205(1), 1993, pp. 149-154
IR lines are calculated for AGN by SVMA code. IR line ratios, as tempe
rature and density diagnostic of the emitting gas, show that the [S II
I] lines ratio increases with shock velocity, following compression an
d cooling of the gas downstream. The results are compared with observa
tions and briefly discussed.