Accretion of gaseous disks of galaxies. I - Influence of dynamical friction on the large-scale H2 distribution

Details Accretion of gaseous disks of galaxies. I - Influence of dynamical friction on the large-scale H2 distribution Accretion of gaseous disks of galaxies. I - Influence of dynamical friction on the large-scale H2 distribution

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987afz....26..363s&link_type=abstract

(Astrofizika, vol. 26, Mar.-Apr. 1987, p. 363-375) Astrophysics (ISSN 0571-7132), vol. 26, no. 2, Sept. 1987, p. 220-228. Transl

Astronomy and Astrophysics

Astrophysics

2

Accretion Disks, Disk Galaxies, Galactic Structure, H Ii Regions, Molecular Clouds, Annuli, Astronomical Models, Friction Factor, Galactic Rotation, Milky Way Galaxy

Scientific paper

The influence of dynamical friction on stars on the global distribution of giant molecular clouds in galaxies is calculated in different model approximations. It is shown that in the Galaxy dynamical friction alone cannot lead to the formation of the observed ring-shaped distribution of the giant molecular clouds during a time comparable with the age of the disk of the Galaxy.

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