SIMBAD references

2004ApJ...613..322Q - Astrophys. J., 613, 322-325 (2004/September-3)

A dynamical model for hot gas in the Galactic Center.

QUATAERT E.

Abstract (from CDS):

Winds from massive stars supply ∼10–3 M/yr of gas to the central parsec of the Galactic center. I present spherically symmetric hydrodynamic simulations of the dynamics of this gas. These calculations show that a few percent of the gas, or ∼fewx10–5 M/yr, flows in toward the central massive black hole Sgr A*; the remaining gas, ∼10–3 M/yr, is thermally driven out of the central star cluster in a wind. This dynamical model accounts for the level of diffuse X-ray emission observed in the central 10" of the Galactic center by Chandra and the extended X-ray source coincident with Sgr A*; the latter is a signature of gas being gravitationally captured by the black hole.

Abstract Copyright:

Journal keyword(s): Accretion, Accretion Disks - Galaxy: Center

Simbad objects: 4

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2020.08.13-02:18:16

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