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The Supernova – ISM/Star-formation interplay

Published online by Cambridge University Press:  29 January 2014

Gerhard Hensler
Gerhard Hensler*
Affiliation:
Department of Astrophysics, University of Vienna, Tuerkenschanzstr. 17, 1180 Vienna, Austria email: gerhard.hensler@univie.ac.at
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Abstract

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Supernovae are the most energetic stellar events and influence the interstellar medium by their gasdynamics and energetics. By this, both also affect the star formation positively and negatively. In this paper, we review the complexity of investigations aiming at understanding the interchange between supernova explosions with the star-forming molecular clouds. Commencing from analytical studies the paper advances to numerical models of supernova feedback from superbubble scales to galaxy structure. We also discuss parametrizations of star-formation and supernova-energy transfer efficiencies. Since evolutionary models from the interstellar medium to galaxies are numerous and are applying multiple recipes of these parameters, only a representative selection of studies can be discussed here.

Keywords

ISM: supernova remnantsISM: kinematics and dynamicsISM: bubblesISM: structurestars: formationgalaxies: evolutiongalaxies: ISM
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S296: Supernova Environmental Impacts , January 2013 , pp. 265 - 272
Copyright
Copyright © International Astronomical Union 2014 

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