Issue EAS Publications Series Volume 10, 2003 JENAM 2002, Galactic & Stellar Dynamics Page(s) 3 DOI 10.1051/eas:2003124

Galactic & Stellar Dynamics
C. Boily, P. Patsis, S. Portegies Zwart, R. Spurzem and C. Theis (eds)
EAS Publications Series, Vol. 10, 2003
DOI: 10.1051/eas:2003124

Gas Dynamics in Central Parts of Galaxies ^*

W. Maciejewski<sup>1, 2

1</sup>  INAF - Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy
²  Obserwatorium Astronomiczne Uniwersytetu Jagiellonskiego, Cracow, Poland

Abstract
Asymmetries in galactic potentials, either self-induced, or caused by a passing companion, play an important role in global gas dynamics in galaxies. In particular, they are able to trigger gas inflow, which in turn feeds nuclear activity. In the inner kiloparsec, the inflowing gas becomes subject to various resonances induced by asymmetry in the potential. This produces complicated gas morphology and dynamics seen in the nuclear rings and spirals. Formation of nuclear rings is related to barred galaxies, and explained by the orbital structure in bars. One can get basic understanding of weak nuclear spirals from the linear wave theory, but stronger spirals are likely to be out of the linear regime, and they appear as spiral shocks in hydrodynamical models. In addition, nuclear stellar bars are observed in a considerable fraction of disc galaxies, often nested inside the large bar; their orbital structure further modifies the nuclear gas dynamics. If a massive black hole (MBH) is present in the galactic centre, it governs the resonances even beyond its classically defined sphere of influence. Since resonances shape gas dynamics in the nuclear region, the central black hole should be able to regulate gas flow around itself.

© EAS, EDP Sciences 2003

What is OpenURL?