Radio Variability Confirmed for SN 2012aw in M95

Details Radio Variability Confirmed for SN 2012aw in M95 Radio Variability Confirmed for SN 2012aw in M95

Apr 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012atel.4012....1s&link_type=abstract

The Astronomer's Telegram, #4012

Astronomy and Astrophysics

Astronomy

Radio, Supernovae

Scientific paper

The Type IIP Supernova 2012aw (CBET #3054) in the galaxy M95 has been observed with the Karl G. Jansky Very Large Array on 2012 Mar 24.25 at frequencies of 20.8 GHz. Radio emission was detected near the supernova location, with a flux density of 0.160 ± 0.025 mJy. This variable radio source is coincident with the detection on 2012 Mar 30.1 of 0.315+/-0.018 mJy (ATEL #4010). The National Radio Astronomy Observatory is facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc.

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