MODEL FOR THE FORMATION OF MOLECULAR CLOUDS IN OUR GALAXY. THE ROLE OF DARK HALO
Numerical gasdynamic model of the galactic gaseous disk taking into account the spiral pattern of the galaxy stellar component is built. The main objective is to study the mechanisms of formation of giant molecular clouds. Comparison of small-scale gaseous structures with observations made. We pose the question of possible influence of the parameters of the dark halo in the characteristic features of giant molecular clouds.