Accretion of Stellar Winds in the Galactic Centre

Details Accretion of Stellar Winds in the Galactic Centre Accretion of Stellar Winds in the Galactic Centre

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006rmxac..26..139c&link_type=abstract

XI IAU Regional Latin American Meeting of Astronomy (Eds. L. Infante & M. Rubio) Revista Mexicana de Astronomía y Astrofísica (S

Astronomy and Astrophysics

Astronomy

Accretion, Accretion Discs, Galaxy: Center, Stars: Winds, Outflows

Scientific paper

Sgr A* is identified with the M_{BH} ˜ 3.5×10^6M&sun; super-massive black hole (SMBH) at the centre of our Galaxy. By virtue of its proximity, Sgr A* may play a key role in the understanding of Active Galactic Nuclei (AGN). Indeed, this is the only AGN where observations detail the origin of the gas in the vicinity of the SMBH. This information is absolutely necessary for the accretion problem to be modelled self-consistently.

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