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dc.contributor.authorAharonian, F.
dc.contributor.authorBüsching, I.
dc.contributor.authorDe Jager, O.C.
dc.contributor.authorHolleran, M.
dc.contributor.authorRaubenheimer, B.C.
dc.contributor.authorVenter, C.
dc.date.accessioned2010-01-08T14:09:38Z
dc.date.available2010-01-08T14:09:38Z
dc.date.issued2008
dc.identifier.citationAharonian F. et al. 2008. Exploring a SNR/molecular cloud association within HESS J1745-303. Astronomy & astrophysics, 483(2):509-517. [http://www.aanda.org/]en
dc.identifier.issn0005-6361
dc.identifier.issn1432-0746 (Online)
dc.identifier.urihttp://hdl.handle.net/10394/2744
dc.identifier.urihttp://dx.doi.org/10.1051/0004-6361:20079230
dc.description.abstractAims. HESS J1745−303 is an extended, unidentified VHE (very high energy) gamma-ray source discovered using HESS in the Galactic Plane Survey. Since no obvious counterpart has previously been found in longer-wavelength data, the processes that power the VHE emission are not well understood. Methods. Combining the latest VHE data with recent XMM-Newton observations and a variety of source catalogs and lower-energy survey data, we attempt to match (from an energetic and positional standpoint) the various parts of the emission of HESS J1745−303 with possible candidates. Results. Though no single counterpart is found to fully explain the VHE emission, we postulate that at least a fraction of the VHE source may be explained by a supernova-remnant/molecular-cloud association and/or a high-spin-down-flux pulsar
dc.description.urihttp://www.aanda.org/index.php?option=article&access=standard&Itemid=129&url=/articles/aa/pdf/2008/20/aa9230-07.pdf
dc.language.isoenen
dc.publisherEDP Sciencesen
dc.titleExploring a SNR/molecular cloud association within HESS J1745-303en
dc.typeArticleen
dc.contributor.researchID10859748 - Holleran, Mathew
dc.contributor.researchID12006653 - Venter, Christo


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