Dark matter in SC galaxies

Details Dark matter in SC galaxies Dark matter in SC galaxies

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aj....106..899o&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 106, no. 3, p. 899-906.

Statistics

Computation

2

Computational Astrophysics, Dark Matter, Spiral Galaxies, Astronomical Models, Galactic Halos, Spatial Distribution, Stellar Rotation

Scientific paper

In this paper the dark matter in spiral galaxies is studied on the basis of models for the stellar velocity dispersion and stellar rotation velocity. The models are based on Satoh's potential-density pairs and the isothermal dark halo. The resulting parameters for the total potential are used to predict the H I rotation curves. We apply the models to the Sc galaxies NGC 6503 and NGC 3198 with the aim of restricting the dark matter distribution in these systems.

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