An Extended Radio Counterpart of TeV J2032+4130?
Astrophysics
2008-11-26 v1
Abstract
We carried out a 5-pointing mosaic observation of TeV J2032+4130 at 1.4 and 4.8 GHz with the VLA in April of 2003. The analysis of the 4.8GHz data indicate weak wispy shell-like radio structure(s) which are at least partially non-thermal. The radio data is compatible with one or more young supernova remnants or perhaps the signature of large scale cluster shocks in this region induced by the violent action of the many massive stars in Cyg OB2.
Keywords
Cite
@article{arxiv.astro-ph/0703017,
title = {An Extended Radio Counterpart of TeV J2032+4130?},
author = {Y. M. Butt and J. A. Combi and J. Drake and J. P. Finley and A. Konopelko and M. Lister and J. Rodriguez and D. Shepherd},
journal= {arXiv preprint arXiv:astro-ph/0703017},
year = {2008}
}
Comments
Proc. 1st GLAST Symp. Feb 5-8, 2007, Stanford CA