Hostname: page-component-78c5997874-dh8gc Total loading time: 0 Render date: 2024-11-10T14:19:22.465Z Has data issue: false hasContentIssue false
  • English
  • Français

Radio supernovae

Published online by Cambridge University Press:  26 January 2006

L.I. Gurvits ,
S. Frey ,
S. Rawlings ,
J. M. Marcaide  and
A. Alberdi
J. M. Marcaide
Affiliation:
Depto. de Astronomía, Universidad de Valencia, 46100 Burjassot, Spain
A. Alberdi
Affiliation:
IAA-CSIC, Apdo. Correos 3004, 18080 Granada, Spain
Get access

Abstract


Only a handful of supernovae can be studied with milliarcsecondresolution using the VLBI technique. However, such rare studieshave permitted in various cases to estimate expansiondecelerations and to obtain information on supernova ejecta andcircumstellar media, as well as on the structure of the emittingregion. We review results on high resolution observations of thenearby radio supernovae: SN 1979C, SN 1986J, SN 1987A, andSN 1993J. For completeness, we also review the results on thesupernova remnants in M 82.


Type
Research Article
Information
European Astronomical Society Publications Series , Volume 15: Radio Astronomy from Karl Jansky to Microjansky – JENAM'03 , 2005 , pp. 207 - 218
Copyright
© EAS, EDP Sciences, 2005

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)