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A Most Energetic Type Ic Supernova: SN 2003L

Soderberg, Alicia M. (2005) A Most Energetic Type Ic Supernova: SN 2003L. In: Cosmic Explosions: On the 10th Anniversary of SN1993J. Springer Proceedings in Physics. No.99. Springer-Verlag , Berlin/Heidelberg, pp. 117-121. ISBN 3540230394. https://resolver.caltech.edu/CaltechAUTHORS:20190829-131533290

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Abstract

We present extensive radio observations of SN2003L, the most luminous and energetic Type Ic radio supernova with the exception of SN 1998bw. Using radio data, we are able to constrain the physical parameters of the supernova, including the velocity and energy of the fastest ejecta, the temporal evolution of the magnetic field, and the density profile of the surrounding medium. We highlight the extraordinary properties of the radio emission with respect to the supernova’s normal characteristics within optical bands. We find that although the explosion does not show evidence for a significant amount of relativistic ejecta, it produces a radio luminosity which is comparable to that seen in the unusual SN1998bw. Using SN2003L as an example, we comment briefly on the broad diversity of type Ic properties and the associated implications for progenitor models.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.1007/3-540-26633-x_15DOIArticle
https://rdcu.be/b3YnVPublisherFree ReadCube access
Additional Information:© Springer-Verlag Berlin Heidelberg 2005.
Series Name:Springer Proceedings in Physics
Issue or Number:99
DOI:10.1007/3-540-26633-x_15
Record Number:CaltechAUTHORS:20190829-131533290
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190829-131533290
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:98344
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:30 Aug 2019 14:20
Last Modified:16 Nov 2021 17:38

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