Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S303(9), p. 174-176, 2013
DOI: 10.1017/s1743921314000489
Full text: Unavailable
AbstractWe 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.