Detection of Radio Transients from Supernovae

Details Detection of Radio Transients from Supernovae Detection of Radio Transients from Supernovae

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21812703s&link_type=abstract

American Astronomical Society, AAS Meeting #218, #127.03; Bulletin of the American Astronomical Society, Vol. 43, 2011

Astronomy and Astrophysics

Astronomy

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. The radio waves emitted are detectable by a new generation of low-frequency radio telescope arrays. We present details of an ongoing search for such events by the Eight-meter-wavelength Transient Array (ETA) and the Long Wavelength Array (LWA).

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