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Shocks, cooling and the origin of star formation rates in spiral galaxies

Abstract. Understanding star formation is problematic as it originates in the large-scale dynamics of a galaxy but occurs on the small scale of an individual st

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Bibliographic Details
Main Authors: Bonnell, Ian (Author) , Dobbs, Clare (Author) , Smith, Rowan J. (Author)
Format: Article (Journal)
Language:English
Published: 18 February 2013
In: Monthly notices of the Royal Astronomical Society
Year: 2013, Volume: 430, Issue: 3, Pages: 1790-1800
ISSN:1365-2966
DOI:10.1093/mnras/stt004
Online Access:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/stt004
Verlag, lizenzpflichtig, Volltext: https://academic.oup.com/mnras/article/430/3/1790/979005
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Author Notes:Ian A. Bonnell, Clare L. Dobbs and Rowan J. Smith
Description
Summary:Abstract. Understanding star formation is problematic as it originates in the large-scale dynamics of a galaxy but occurs on the small scale of an individual st
Item Description:Gesehen am 02.12.2020
Physical Description:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/stt004

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