Strong radio emission from SN 2007bg one year after the explosion - detection of spreading, off-axis GRB jet?

Details Strong radio emission from SN 2007bg one year after the explosion - detection of spreading, off-axis GRB jet? Strong radio emission from SN 2007bg one year after the explosion - detection of spreading, off-axis GRB jet?

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009atel.2065....1p&link_type=abstract

The Astronomer's Telegram, #2065

Astronomy and Astrophysics

Astronomy

1

Radio, Request For Observations, Novae, Supernovae

Scientific paper

In their study of supernova hosts using SDSS data (Prieto, Stanek & Beacom 2008, ApJ, 673, 999), the broad-lined SN Ic 2007bg at z=0.034 (Quimby et al. 2007, #CBET 927; Harutyunyan et al. 2007, CBET #948; Soderberg & Immler 2007, ATEL #1142), was identified as a good candidate for an off-axis GRB. The likely host of SN 2007bg is an extremely low- luminosity galaxy with M_B ~ -12, one of the least-luminous supernova hosts of any kind ever observed.

Affiliated with

Also associated with

No associations

Rating

Strong radio emission from SN 2007bg one year after the explosion - detection of spreading, off-axis GRB jet? does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Strong radio emission from SN 2007bg one year after the explosion - detection of spreading, off-axis GRB jet?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Strong radio emission from SN 2007bg one year after the explosion - detection of spreading, off-axis GRB jet? will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-807146