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Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/105756
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dc.contributor.authorVoisin, F.-
dc.contributor.authorRowell, G.-
dc.contributor.authorBurton, M.-
dc.contributor.authorFukui, Y.-
dc.contributor.authorSano, H.-
dc.contributor.authorAharonian, F.-
dc.contributor.editorAharonian, F.-
dc.contributor.editorHofmann, W.-
dc.contributor.editorRieger, F.-
dc.date.issued2017-
dc.identifier.citationAIP Conference Proceedings, 2017 / Aharonian, F., Hofmann, W., Rieger, F. (ed./s), vol.1792, pp.040011-1-040011-6-
dc.identifier.isbn9780735414563-
dc.identifier.issn0094-243X-
dc.identifier.issn1551-7616-
dc.identifier.urihttp://hdl.handle.net/2440/105756-
dc.description.abstractPulsar wind Nebulae (PWNe) represent the largest population of TeV sources detected by H.E.S.S. Here, we present a ISM study combining 7mm Mopra observations with Nanten CO(1–0) and SGPS Hi data to understand the ISM environment towards HESS J1809−193, HESS J1026−582 and HESS J1826−130, as well as the morphology of the TeV source gamma-ray emission. Combining the TeV emission with several extended dense regions will then be useful to quantify the distinguish the contribution from PWNe and SNRs towards various HESS TeV sources.-
dc.description.statementofresponsibilityF. Voisin, G. Rowell, M. G. Burton, Y. Fukui, H. Sano and F. Aharonian-
dc.language.isoen-
dc.publisherAmerican Institute of Physics-
dc.relation.ispartofseriesAIP Conference Proceedings-
dc.rights© The author. © AIP Publishing LLC Proceedings issue.-
dc.source.urihttp://dx.doi.org/10.1063/1.4968915-
dc.titleISM studies towards several PWNe-
dc.typeConference paper-
dc.contributor.conference6th International Meeting on High Energy Gamma-Ray Astronomy (11 Jul 2016 - 15 Jul 2016 : Heidelberg, Germany)-
dc.identifier.doi10.1063/1.4968915-
pubs.publication-statusPublished-
dc.identifier.orcidRowell, G. [0000-0002-9516-1581]-
Appears in Collections:Aurora harvest 8
Physics publications

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