Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4145
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dc.contributor.authorOsborne, J.-
dc.contributor.authorPandey-Pommier, M.-
dc.contributor.authorUdaya Shankar, N.-
dc.date.accessioned2011-08-24T05:46:02Z-
dc.date.available2011-08-24T05:46:02Z-
dc.date.issued2009-09-
dc.identifier.citationASP Conference Series, 2009, Vol.407, p349en
dc.identifier.urihttp://hdl.handle.net/2289/4145-
dc.descriptionOpen Access. Proceedings of the conference held 8-12 December 2008, at National Centre for Radio Astrophysics (NCRA), TIFR, Pune, India. Edited by D. J. Saikia, D. A. Green, Y. Gupta, and T. Venturi. San Francisco: Astronomical Society of the Pacific.en
dc.description.abstractWe have observed 4 VHE gamma-ray sources discovered by the High Energy Stereoscopic System (H.E.S.S.) with the Giant Metrewave Radio Telescope (GMRT). The sources viz., HESS J1813-178, HESS J1825-137, HESS J1834-087, and HESS J1837-069 were observed simultaneously at 0.61 and 0.235 GHz and at 1.28 GHz. Resolved source counterparts for 3 of these were detected at all the three frequencies. None was detected for HESS J1825-137. We investigate the consistent multiwavelength behaviour of these sources and plausible gamma-ray emission mechanisms.en
dc.language.isoenen
dc.publisherAstronomical Society of the Pacificen
dc.relation.urihttp://adsabs.harvard.edu/abs/2009ASPC..407..349Oen
dc.rights2009 Astronomical Society of the Pacific.en
dc.titleGMRT observations of H.E.S.S. sourcesen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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