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C. J. Stockdale (NRL/NRC), R. A. Sramek (NRAO), K .W. Weiler (NRL), S. D. Van Dyk (IPAC/CIT), M. A. Perez-Torres (Istituto di Radioastronomia, Bologna), J. M. Marcaide (University of Valencia), A. Ray, P. Chandra (Tata Institute of Fundamental Research, Mumbai), N. Panagia (ESA/STSI), M. J. Montes (NRL)
We present results from the on-going radio monitoring of Supernova 2001gd in NGC 5033. Using the Very Large Array (VLA) and the Giant Meterwave Radio Telescope (GMRT) to monitor the supernova at 1.3, 2, 3.6, 6, 20 and 90 cm, we present radio light-curves of this type IIb supernova. We discuss parameterizations and modelling of this data and make predictions for the continuing evolution of this source.
The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. C. J. Stockdale is a NRC Postdoctoral Fellow.
The author(s) of this abstract have provided an email address for comments about the abstract: stockdale@nrl.navy.mil
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Bulletin of the American Astronomical Society, 34, #4
© 2002. The American Astronomical Soceity.