Flat rotational curves without dark matter

Details Flat rotational curves without dark matter Flat rotational curves without dark matter

2006-11-09

arxiv.org/abs/astro-ph/0611303v1

Astronomy and Astrophysics

Astrophysics

10 pages

Scientific paper

We consider the singular configurations of gravitating gas [1] which could be
used as a model for disk galaxies. The simplest steady configuration, which
corresponds to rotation of stars around center gives flat rotational curve,
provided the density distrubution has a tail, decaying as 1/r. This result
based exclusively on Newtonian gravity and does not involve dark matter.

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