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 super massive black hole.
@article{arxiv.1311.2738,
title = {Galactic Dynamics feeding the Galactic Center},
author = {Florent Renaud and Eric Emsellem and Frédéric Bournaud},
journal= {arXiv preprint arXiv:1311.2738},
year = {2015}
}
Comments
Proceedings of the IAU Symposium 303 "The Galactic Center: Feeding and Feedback in a Normal Galactic Nucleus"