An Extended Radio Counterpart of TeV J2032+4130?

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dc.creatorButt, Y. M.
dc.creatorCombi, J. A.
dc.creatorDrake, J.
dc.creatorFinley, J. P.
dc.creatorKonopelko, A.
dc.creatorLister, M.
dc.creatorRodriguez, J.
dc.creatorShepherd, D.
dc.date2007-03-01
dc.date.accessioned2026-07-07T10:36:54Z
dc.date.available2026-07-07T10:36:54Z
dc.descriptionWe 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.
dc.descriptionProc. 1st GLAST Symp. Feb 5-8, 2007, Stanford CA
dc.identifierhttps://arxiv.org/abs/astro-ph/0703017
dc.identifierhttp://arxiv.org/abs/astro-ph/0703017
dc.identifierAIPConf.Proc.921:429-430,2007
dc.identifierdoi:10.1063/1.2757386
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/180208
dc.subjectAstrophysics
dc.titleAn Extended Radio Counterpart of TeV J2032+4130?
dc.typetext

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