The radio luminous SN 2007bg: evidence for circumstellar interaction

Details The radio luminous SN 2007bg: evidence for circumstellar interaction The radio luminous SN 2007bg: evidence for circumstellar interaction

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009atel.2066....1s&link_type=abstract

The Astronomer's Telegram, #2066

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4

Radio, Gamma-Ray Bursts, Novae, Supernovae

Scientific paper

Through our on-going Very Large Array program dedicated to the study of radio emission from Type Ibc supernovae, we have obtained extensive multi-frequency observations of SN2007bg throughout the two years since its optical discovery (Quimby et al. CBET #927). Over this timescale, the SN shows detectable radio emission with a luminosity somewhat higher than that of other radio luminous SNe, including the Type Ibc SN 2003L (Soderberg et al.

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