Abstract
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. Copyright © International Astronomical Union 2014.
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CITATION STYLE
APA
Renaud, F., Emsellem, E., & Bournaud, F. (2014). Galactic dynamics feeding the Galactic center. Proceedings of the International Astronomical Union, 9(S303), 174–176. https://doi.org/10.1017/S1743921314000489
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