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Supernova Remnants in Starburst Regions

Published online by Cambridge University Press:  21 March 2013

A. I. Asvarov
A. I. Asvarov*
Affiliation:
Institute of Physics, Baku AZ1143, Azerbaijan. email: [email protected]
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Abstract

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We study the evolution of SNRs in starburst regions taking into consideration the role of the high ambient pressure and the influence of gravitational forces from the stellar component within the shell of a SNR. On this basis, we discuss the connection between the radio, infrared, and gamma emissions from starburst regions.

Keywords

supernova remnants — galaxies: starburst
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S292: Molecular Gas, Dust, and Star Formation in Galaxies , August 2012 , pp. 97
Copyright
Copyright © International Astronomical Union 2013

References

Draine, B. T. & Woods, D. T. 1991, ApJ, 383, 621CrossRefGoogle Scholar
Storm, M. E., Jeltema, E. T., & Profumo, S. 2012, arXiv:1206.1676v1Google Scholar