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Optical, Ultraviolet, and Infrared Observations of SN 1993J

Published online by Cambridge University Press:  19 September 2016

Alexei V. Filippenko  and
Thomas Matheson
Alexei V. Filippenko
Affiliation:
Department of Astronomy, University of California, 601 Campbell Hall, Berkeley, CA 94720-3411, USA; alex@astron.berkeley.edu
Thomas Matheson
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USAtmatheson@cfa.harvard.edu

Summary

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We review the existing set of optical/UV/IR observations of Supernova 1993J, concentrating heavily on optical data because these are by far the most plentiful. Some results from theoretical modeling of the observations are also discussed. SN 1993J has provided the best observational evidence for the transformation of a SN from one spectral type to another, thereby providing a link between Type II and Type Ib supernovae (SNe). This has strengthened the argument that SNe Ib (and, by extension, SNe Ic) are core-collapse events. SN 1993J has remained relatively bright for 10 years; its late-time emission comes from the collision of supernova ejecta with circumstellar gas that was released by the progenitor prior to the explosion. The circumstellar material shows strong evidence of CNO processing.

Type
Part I Supernovae: Individual
Information
International Astronomical Union Colloquium , Volume 192: Cosmic Explosions , 2005 , pp. 37 - 46
Copyright
Copyright © Springer-Verlag 2005

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