Note to users. If you're seeing this message, it means that your browser cannot find this page's style/presentation instructions -- or possibly that you are using a browser that does not support current Web standards. Find out more about why this message is appearing, and what you can do to make your experience of our site the best it can be.


Science 1 December 1995:
Vol. 270. no. 5241, pp. 1475 - 1478
DOI: 10.1126/science.270.5241.1475

Reports

Expansion of SN 1993J

J. M. Marcaide (1),  A. Alberdi,  E. Ros,  P. Diamond,  I. I. Shapiro,  J. C. Guirado,  D. L. Jones,  T. P. Krichbaum,  F. Mantovani,  R. A. Preston,  A. Rius,  R. T. Schilizzi,  C. Trigilio,  A. R. Whitney,  A. Witzel

A sequence of images from very long baseline interferometry shows that the young radio supernova SN 1993J is expanding with circular symmetry. However, the circularly symmetric images show emission asymmetries. A scenario in which freely expanding supernova ejecta shock mostly isotropic circumstellar material is strongly favored. The sequence of images constitutes the first ``movie'' of a radio supernova.


J. M. Marcaide and E. Ros, Departamento de Astronomía, Universitat de València, E-46100 Burjassot, València, Spain.
A. Alberdi, Laboratorio de Astrofísica Espacial y Física Fundamental, Instituto Nacional de Técnica Aeroespacial (INTA), E-28080 Madrid, Spain, and Instituto de Astrofísica de Andalucía-Consejo Superior de Investigaciones Cientificas (CSIC), Apdo. Correos 3004, E-18080 Granada, Spain.
P. Diamond, National Radio Astronomy Observatory, Socorro, NM 87801, USA.
I. I. Shapiro, Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA.
J. C. Guirado, D. L. Jones, R. A. Preston, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.
T. P. Krichbaum and A. Witzel, Max-Planck Institut für Radioastronomie, Auf dem Hügel 69, D-50131 Bonn, Germany.
F. Mantovani, Istituto di Radioastronomia, Consiglio Nazionale delle Ricerche (CNR), I-Bologna 40129, Italy.
A. Rius, Laboratorio de Astrofísica Espacial y Física Fundamental, INTA, E-28080 Madrid, Spain, and Centre d'Estudis Avançats-C.S.I.C., Camí de Santa Barbara s/n, E-17300 Blanes, Girona, Spain.
R. T. Schilizzi, Joint Institute for VLBI in Europe, Postbus 2, 7990 AA Dwingeloo, Netherlands, and Leiden Observatory, Postbus 9513, 2300 RA Leiden, Netherlands.
C. Trigilio, Istituto di Radioastronomia, CNR, Noto, Italy.
A. R. Whitney, Massachusetts Institute of Technology-Haystack Observatory, Westford, MA 01886, USA.
(1) To whom correspondence should be addressed.


THIS ARTICLE HAS BEEN CITED BY OTHER ARTICLES:
The Changing Morphology and Increasing Deceleration of Supernova 1993J in M81.
N. Bartel, M. F. Bietenholz, M. P. Rupen, A. J. Beasley, D. A. Graham, V. I. Altunin, T. Venturi, G. Umana, W. H. Cannon, and J. E. Conway (2000)
Science 287, 112-116
   Abstract »    Full Text »
Type II Supernovae SN 1987A and SN 1993J.
R. A. Chevalier (1997)
Science 276, 1374-1378
   Abstract »    Full Text »
An Exploding Star in Motion.
R. A. Chevalier (1995)
Science 270, 1452-1453
   Abstract »    PDF »



To Advertise     Find Products


Science. ISSN 0036-8075 (print), 1095-9203 (online)