Consideration of the general expansion of the Galaxy in studies of the dependence of the neutral hydrogen subsystem rotation velocity on the Z coordinate

Details Consideration of the general expansion of the Galaxy in studies of the dependence of the neutral hydrogen subsystem rotation velocity on the Z coordinate Consideration of the general expansion of the Galaxy in studies of the dependence of the neutral hydrogen subsystem rotation velocity on the Z coordinate

Jul 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986velen.......78b&link_type=abstract

Leningradskii Universitet, Vestnik, Matematika, Mekhanika, Astronomiia (ISSN 0024-0850), July 1986, p. 78-83. In Russian.

Astronomy and Astrophysics

Astronomy

Galactic Rotation, Hydrogen Clouds, Milky Way Galaxy, Neutral Gases, Angular Velocity, Astronomical Coordinates, Radio Astronomy

Scientific paper

A method is proposed for determining the dependence of the angular rotation velocity of the neutral hydrogen subsystem on the z coordinate from observational data at 21 cm with allowance for the general expansion of the Galaxy. The method is based on a generalization of a purely rotational model of a hydrogen layer allowing for the angular velocity dependence. The analysis considers the internal (with respect to the sun) regions of the Galaxy.

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