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Light Curves of Radio Supernovae

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Other literature type 01 Jan 2007Embargo end date: 01 Jan 2007Publisher:AIPJournal:AIP Conference Proceedings (issn: 0094-243X,

Authors: M. T. Kelley; C. J. Stockdale; K. W. Weiler; C. L. M. Williams; N. Panagia; R. A. Sramek; J. M. Marcaide; +3 Authors

doi: 10.1063/1.3682913 , 10.1063/1.2803574 , 10.48550/arxiv.0708.1180

arXiv: http://arxiv.org/abs/0708.1180

Light Curves of Radio Supernovae

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Abstract

We present the results from the on-going radio monitoring of recent type II supernovae (SNe), including SNe 2004et, 2004dj, 2002hh, 2001em, and 2001gd. Using the Very Large Array to monitor these supernovae, we present their radio light-curves. From these data we are able to discuss parameterizations and modeling and make predictions of the nature of the progenitors based on previous research. Derived mass loss rates assume wind-established circumstellar medium, shock velocity ~10,000 km/s, wind velocity ~10 km/s, and CSM Temperature ~10,000 K.

3 pages, 6 figures Conference Proceedings: "Supernova 1987A: 20 Years After: Supernovae and Gamma-Ray Bursters" AIP, New York, eds. S. Immler, K.W. Weiler, and R. McCray

Related Organizations

California Institute of Technology
United States
National Radio Astronomy Observatory
United States
Space Telescope Science Institute
United States
Massachusetts Institute of Technology
United States
Marquette University
United States

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Keywords

Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

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