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Radio Observations Of A Nearby Type IIP SN 2012aw

Published online by Cambridge University Press:  29 January 2014

Naveen Yadav
Affiliation:
Tata Institute of Fundamental Research, Mumbai, India email: naveen.phys@gmail.com
Alak Ray
Affiliation:
Tata Institute of Fundamental Research, Mumbai, India email: naveen.phys@gmail.com
Sayan Chakraborti
Affiliation:
Harvard-Smithsonian CfA, USA
Christopher Stockdale
Affiliation:
Marquette University, USA
Poonam Chandra
Affiliation:
National Center for Radio Astronomy-TIFR, India
Randall Smith
Affiliation:
Harvard-Smithsonian CfA, USA
Rupak Roy
Affiliation:
Aryabhhata Research Institute of Observational Sciences, India
Vikram Dwarkadas
Affiliation:
University of Chicago, USA
Firoza Sutaria
Affiliation:
Indian Institute of Astrophysics, India
Dave Pooley
Affiliation:
Sam Houston State University, Huntsville, USA
Brijesh Kumar
Affiliation:
Aryabhhata Research Institute of Observational Sciences, India
Subhash Bose
Affiliation:
Aryabhhata Research Institute of Observational Sciences, India
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Abstract

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SN 2012AW is a type-IIP supernova which exploded in M95. In this paper we discuss the radio observations of this supernova and model them to determine the important parameters relevant to the explosion and the evolution of blast wave. We also determine the dominant cooling process important to this source.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2014 

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