Observations of the bright radio transient in M82: a new radio supernova?

Details Observations of the bright radio transient in M82: a new radio supernova? Observations of the bright radio transient in M82: a new radio supernova?

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009atel.2060....1b&link_type=abstract

The Astronomer's Telegram, #2060

Astronomy and Astrophysics

Astronomy

6

Radio, Novae, Supernovae

Scientific paper

We report MERLIN radio observations of the recently announced radio transient and supernova candidate in M82. The radio transient was first detected on 2008 March 24 and reported by Brunthaler et al 2009 (ATEL#2020 & arXiv:0904.2388). Analysis of MERLIN observations taken between 1200UT 1st May and 1600UT 3rd May 2008 4994MHz shows the source to have a mean flux density of 117mJy. Over the duration of this observation the flux density of the new source increased from ~113mJy to ~119mJy.

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