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Deceleration in the Expansion of SN 1993J

Published online by Cambridge University Press:  12 April 2016

J. M. Marcaide
Affiliation:
Departamento de Astronomía, Universitat de València, E-46100 Burjassot, Spain
A. Alberdi
Affiliation:
LAEFF-INTA, 28080 Madrid, Spain IAA-CSIC, 18080 Granada, Spain
E. Ros
Affiliation:
Departamento de Astronomía, Universitat de València, E-46100 Burjassot, Spain
P. Diamond
Affiliation:
NRAO, Socorro, NM 87801, USA
I. I. Shapiro
Affiliation:
Harvard-Smithsonian CfA, Cambridge, MA 02138, USA
J. C. Guirado
Affiliation:
Departamento de Astronomía, Universitat de València, E-46100 Burjassot, Spain
D.L. Jones
Affiliation:
JPL, Pasadena, CA 91109, USA
F. Mantovani
Affiliation:
IRA-CNR, Bologna 40129, Italy
M. A. Pérez-Torres
Affiliation:
Departamento de Astronomía, Universitat de València, E-46100 Burjassot, Spain
R. A. Preston
Affiliation:
JPL, Pasadena, CA 91109, USA
R. T. Schilizzi
Affiliation:
JIVE, 7990 AA Dwingeloo, Netherlands Leiden Observatory, 2300 RA Leiden, Netherlands
R. A. Sramek
Affiliation:
NRAO, Socorro, NM 87801, USA
C. Trigilio
Affiliation:
IRA-CNR, Noto, Italy
S.D. Van Dyk
Affiliation:
UCLA, Los Angeles, CA 90095
K. W. Weiler
Affiliation:
NRL, Washington, DC 20375-5320
A. R. Whitney
Affiliation:
MIT-Haystack Observatory, Westford, MA 01886, USA

Abstract

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With new 6 cm observations we confirm the self-similar expansion of SN 1993J previously discovered at 3.6 cm and estimate the expansion deceleration parameter. The results are inconsistent with the existence of a constant pre-explosion stellar wind but otherwise confirm the standard radio supernova model. The first map at 13 cm showing shell structure is also presented.

Type
Research Article
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

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