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Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/39765
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dc.contributor.authorRowell, G.en
dc.contributor.authorBerge, D.en
dc.contributor.authorHinton, J.en
dc.date.issued2005en
dc.identifier.citation29th International Cosmic Ray Conference, August 3-10, 2005, Pune, India: [volume 4] / pp. 101-106en
dc.identifier.urihttp://hdl.handle.net/2440/39765-
dc.description.abstractOver the past few years, H.E.S.S. has observed a number of shell-type supernova remnants (SNRs) in order to determine if they are capable of multi-TeV particle acceleration. Apart from RX J1713.7-3946 and RX J0852.0-4622 (Vela Junior) discussed separately at this conference, other candidates such as W28, SN 1987A, IC-443, Monoceros Loop/Rosette Nebula and SN 1006 are among several highly-ranked targets, based on previous TeV results and/or multi-wavelength information. We briefly outline the motivation for these H.E.S.S. observations and summarise details of several candidates.en
dc.description.statementofresponsibilityG.P. Rowell, D. Berge, J.A. Hinton, for the H.E.S.S. Collaborationen
dc.language.isoenen
dc.publisherTata Institute of Fundamental Researchen
dc.titleH.E.S.S. Observations of Shell Type SNRen
dc.typeConference paperen
dc.contributor.conferenceInternational Cosmic Ray Conference (29th : 2005 : Pune, India)en
pubs.publication-statusPublisheden
dc.identifier.orcidRowell, G. [0000-0002-9516-1581]en
Appears in Collections:Aurora harvest
Physics publications

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