Determining the surface density distribution in massive galactic disks with a central black hole

Details Determining the surface density distribution in massive galactic disks with a central black hole Determining the surface density distribution in massive galactic disks with a central black hole

2002-09-11

arxiv.org/abs/astro-ph/0209200v3

Astronomy and Astrophysics

Astrophysics

10 pages, 2 figures; contains the proof corrections and 8 new references; to be published in Astronomy Lett

Scientific paper

10.1134/1.1544528

An efficient method is developed which allows the calculation of distributions of the surface density in the equilibrium disk configurations with an isolated point mass at the center corresponding to known distributions of the angular velocity. We demonstrate the existence of the upper limit for the ratio `mass of the galactic disk / mass of the central black hole' which essentially depends on the form of rotation-curves.

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