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A dynamical model for gas flows, star formation and nuclear winds in galactic centres

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We present a dynamical model for gas transport, star formation and winds in the nuclear regions of galaxies, focusing on the Milky Way's Central Molecular Zone (CMZ). In our model angular momentum and mass are transported by a combination of gravitational and bar-driven acoustic instabilities....

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Main Authors: Krumholz, Mark R. (Author) , Kruijssen, Diederik (Author) , Crocker, Roland M. (Author)
Format: Article (Journal)
Language:English
Published: 10 December 2016
In: Monthly notices of the Royal Astronomical Society
Year: 2017, Volume: 466, Issue: 1, Pages: 1213-1233
ISSN:1365-2966
DOI:10.1093/mnras/stw3195
Online Access:Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1093/mnras/stw3195
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Author Notes:Mark R. Krumholz, J.M. Diederik Kruijssen and Roland M. Crocker
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A dynamical model for gas flows, star formation, and nuclear winds in galactic centres by Krumholz, Mark R. (Author) , Kruijssen, Diederik (Author) , Crocker, Roland M. (Author) ,


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