High-resolution radio imaging of young supernovae
Astrophysics
2007-05-23 v2
Abstract
The high resolution obtained through the use of VLBI gives an unique opportunity to directly observe the interaction of an expanding radio supernova with its surrounding medium. We present here results from our VLBI observations of the young supernovae SN 1979C, SN 1986J, and SN 2001gd.
Keywords
Cite
@article{arxiv.astro-ph/0403273,
title = {High-resolution radio imaging of young supernovae},
author = {M. A. Perez-Torres and J. M. Marcaide and A. Alberdi and E. Ros and J. C. Guirado and L. Lara and F. Mantovani and C. J. Stockdale and K. W. Weiler and P. J. Diamond and S. D. Van Dyk and P. Lundqvist and N. Panagia and I. I. Shapiro and R. Sramek},
journal= {arXiv preprint arXiv:astro-ph/0403273},
year = {2007}
}
Comments
8 pages, 3 figures. Uses svmult.cls. To appear in proceedings of IAU Colloquium 192 "Supernovae (10 years of SN 1993J)", April 2003, Valencia, Spain, eds. J. M. Marcaide and K. W. Weiler