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An Extended Radio Counterpart of TeV J2032+4130?

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arxiv astro-ph/0703017 v1 pith:RH2ZPQFY submitted 2007-03-01 astro-ph

Y. M. Butt , J. A. Combi , J. Drake , J. P. Finley , A. Konopelko , M. Lister , J. Rodriguez , D. Shepherd This is my paper · ORCID
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keywords radiodataj2032actionanalysisaprilcarriedcluster
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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.

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