Recent Type II Radio Supernovae

Details Recent Type II Radio Supernovae Recent Type II Radio Supernovae

Feb 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006sgrb.confe..57s&link_type=abstract

Presented at the KITP Conference: Supernova and Gamma-Ray Burst Remnants, Feb 10, 2006, Kavli Institute for Theoretical Physics,

Physics

Scientific paper

We present results from the on-going radio monitoring of recent type IIsupernovae (SNe), including SNe 2005cs, 2004et, 2004dj, 2003ed, 2002hh,2001em, and 2001gd. Using the Very Large Array (VLA) to monitor thesesupernovae at 1.3, 2, 3.6, 6 and 20 cm, we present their radiolight-curves.From these data we are able to discuss parameterizations and modeling andmake predictions of the nature of the progenitors based on previousresearch. The National Radio Astronomy Observatory is a facility of theNational Science Foundation operated under cooperative agreement byAssociated Universities, Inc. Matthew Kelley and Brian Kaster areundergraduates at Marquette University. KWW thanks the Office of NavalResearch for the 6.1 funding which supports his research.

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