Molecular Clouds Close to the Galactic Center

Simple item page
dc.creatorBiermann, Peter L.
dc.creatorDuschl, Wolfgang J.
dc.creatorvon Linden, Susanne
dc.date1993-05-12
dc.date.accessioned2026-07-07T02:18:46Z
dc.date.available2026-07-07T02:18:46Z
dc.descriptionWe 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 $ν$ is shown to be weakly dependent on the radius $s$: $ν\sim s^{0.4}$. Finally, we discuss the influence of the inner boundary on the structure of the inner disk regions.
dc.description10 pages Plain TeX (using PostScript fonts) Max-Planck-Institut fuer Radioastronomie Preprint Series No. 525 April 1993
dc.identifierhttps://arxiv.org/abs/astro-ph/9305013
dc.identifierhttp://arxiv.org/abs/astro-ph/9305013
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9618
dc.subjectAstrophysics
dc.titleMolecular Clouds Close to the Galactic Center
dc.typetext

Files

Collections

arXiv