A simple model to fit rotation curves.

Details A simple model to fit rotation curves. A simple model to fit rotation curves.

Oct 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993rmxaa..25..111m&link_type=abstract

Revista Mexicana de Astronomia y Astrofisica, Vol. 25, No. 2, p. 111 - 115

Astronomy and Astrophysics

Astronomy

Rotation Curves: Galaxies, Rotation Curves: Stellar Systems

Scientific paper

The authors study analytically a very simple model of mass distribution in flat galaxies, consisting of a flattened spheroid and a spherical bulge, both components being inhomogeneous. The authors show direct fits of the analytically derived rotation curves with some types of observationally obtained rotation curves. A comparison is made with the maximum-disk solution without a halo obtained by Kent (1986).

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