On the Azimuthal Average Distribution of HI in Galaxies

Details On the Azimuthal Average Distribution of HI in Galaxies On the Azimuthal Average Distribution of HI in Galaxies

Nov 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987atsir1519....1z&link_type=abstract

Astronomicheskii Tsirkulyar NO. 1519/NOV, P. 1, 1987

Astronomy and Astrophysics

Astronomy

1

Scientific paper

It is shown that radius RH of maximal density of H I in
galaxies is closely related to the radius Rv where the
rotation curve reaches "plateau". This may be a consequence of
development of shear instability of gaseous discs with non-monotonous
character of V(R).

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