Electromagnetic Transients from Supernovae

Details Electromagnetic Transients from Supernovae Electromagnetic Transients from Supernovae

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aps..apr.c1017k&link_type=abstract

American Physical Society, APS April Meeting 2010, February 13-16, 2010, abstract #C1.017

Physics

Scientific paper

A core-collapse supernova (SN) would produce an expanding shell of charged particles which interact with the surrounding magnetic field of the progenitor star producing a transient radio pulse. Approximately one supernova event per century is expected in a galaxy. Such a pulse may be detected by a transient radio array. We present details of an ongoing such for such events by the Eight-meter-wavelength Transient Array (ETA). )

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