Astronomy and Astrophysics – Astrophysics
Scientific paper
Jan 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...209...46t&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 209, no. 1-2, Jan. 1989, p. 46-50.
Astronomy and Astrophysics
Astrophysics
6
Centimeter Waves, Galactic Rotation, Hydrogen, Line Spectra, Neutral Gases, Galactic Structure, H I Regions, Milky Way Galaxy
Scientific paper
A graphic variation of the Agekyan et al. (1964) method for investigating the galactic rotation curve from whole H-I 21-cm line profiles has been applied to distances to the galactic center, R, smaller than that of the sun, R(0). The results are consistent with an axisymmetric distribution of H I. The points of the rotation curve for R/R(0) values of between 0.4 and 1 are found to be 5-10 km/s below the usual rotation curve obtained from tangential points.
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