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VLBI Observations of Supernova 1993J: The First 1000 Days

Published online by Cambridge University Press:  12 April 2016

M. P. Rupen ,
A. J. Beasley ,
N. Bartel ,
M. F. Bietenholz ,
D. A. Graham ,
V. I. Altunin ,
D. L. Jones ,
J. E. Conway ,
T. Venturi  and
G. Umana
...Show all authors
M. P. Rupen
Affiliation:
National Radio Astronomy Observatory, Socorro, NM 87801, U.S.A.
A. J. Beasley
Affiliation:
National Radio Astronomy Observatory, Socorro, NM 87801, U.S.A.
N. Bartel
Affiliation:
York University, North York, ONT M3J 1P3, Canada
M. F. Bietenholz
Affiliation:
York University, North York, ONT M3J 1P3, Canada
D. A. Graham
Affiliation:
Max-Planck-Institut für Radioastronomie, Postfach 2024, 53010 Bonn, Germany
V. I. Altunin
Affiliation:
Jet Propulsion Laboratory, Pasadena, CA 91009, U.S.A.
D. L. Jones
Affiliation:
Jet Propulsion Laboratory, Pasadena, CA 91009, U.S.A.
J. E. Conway
Affiliation:
Onsala Space Observatory, Onsala, Sweden
T. Venturi
Affiliation:
Istituto di Radioastronomia, 40129 Bologna, Italy
G. Umana
Affiliation:
Istituto di Radioastronomia, 96017 Noto (SR), Italy
A. Rius
Affiliation:
Centro de Estudios Avanzados de Blanes, Blanes, Spain

Abstract

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We report on phase-referenced 5 and 8.4 GHz VLBI images of supernova SN 1993J in M81, tracking the evolution of the source from 50 to 1000 days after the explosion.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 164: Radio Emission from Galactic and Extragalactic Compact Sources , 1998 , pp. 355 - 356
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

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