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Peering into the heart of the M82 starburst

Published online by Cambridge University Press:  27 October 2016

Danielle Fenech ,
Tom Muxlow ,
Rob Beswick  and
Megan Argo
Danielle Fenech
Affiliation:
Department of Physics and Astronomy, University College London, Gower Street, London, WC1E 6BT, U.K. email: dmf@star.ucl.ac.uk
Tom Muxlow
Affiliation:
Jodrell Bank Centre for Astrophysics, The University of Manchester, U.K.
Rob Beswick
Affiliation:
Jodrell Bank Centre for Astrophysics, The University of Manchester, U.K.
Megan Argo
Affiliation:
Jodrell Bank Centre for Astrophysics, The University of Manchester, U.K.
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Abstract

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We present multi-epoch millarcsecond resolution images of the most compact supernova remnants in the nearby starburst galaxy M82, spanning 25 years of evolution. In particular, we will briefly discuss the new transient source first detected in 2009 as well as the unusual object 41.95+57.5 and its potential as a GRB afterglow.

Keywords

radio continuum: supernova remnantstechniques: interferometrichigh angular resolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , General Assembly A29B: Astronomy in Focus , August 2015 , pp. 233 - 234
Copyright
Copyright © International Astronomical Union 2016 

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