Molecular Clouds Close to the Galactic Center

Details Molecular Clouds Close to the Galactic Center Molecular Clouds Close to the Galactic Center

1993-05-12

arxiv.org/abs/astro-ph/9305013v1

Astronomy and Astrophysics

Astrophysics

10 pages Plain TeX (using PostScript fonts) Max-Planck-Institut fuer Radioastronomie Preprint Series No. 525 April 1993

Scientific paper

We demonstrate that the accretion disk model for the Galactic Center region by Linden et al (1993a) is applicable for at least one order of magnitude in radius from the Galactic Center (10 ... 100 pc). The viscosity $\nu$ is shown to be weakly dependent on the radius $s$: $\nu \sim s^{0.4}$. Finally, we discuss the influence of the inner boundary on the structure of the inner disk regions.

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