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Galactic dynamics feeding the Galactic center

Published online by Cambridge University Press:  22 May 2014

Florent Renaud ,
Eric Emsellem  and
Frédéric Bournaud
Florent Renaud
Affiliation:
Laboratoire AIM Paris-Saclay, CEA/IRFU/SAp, Université Paris Diderot, F-91191 Gif-sur-Yvette Cedex, France email: florent.renaud@cea.fr
Eric Emsellem
Affiliation:
European Southern Observatory, 85748 Garching bei Muenchen, Germany Université Lyon 1, Observatoire de Lyon, CRAL et ENS, 9 Av Charles André, F-69230 Saint-Genis Laval, France
Frédéric Bournaud
Affiliation:
Laboratoire AIM Paris-Saclay, CEA/IRFU/SAp, Université Paris Diderot, F-91191 Gif-sur-Yvette Cedex, France email: florent.renaud@cea.fr
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Abstract

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We present the hierarchical structure of the gas and its rapid evolution in the central region of a simulation of the entire Milky Way, run at subparsec resolution. We emphasize the coupling between the kpc-scale dynamics, the molecular ring and the central 5 pc disk feeding the supermassive black hole.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S303: The Galactic Center: Feeding and Feedback in a Normal Galactic Nucleus , October 2013 , pp. 174 - 176
Copyright
Copyright © International Astronomical Union 2014 

References

Renaud, F., et al. 2013, MNRAS, in press, arXiv:1307.5639Google Scholar
Teyssier, R. 2002, A&A 385, 337Google Scholar