Please use this identifier to cite or link to this item: http://hdl.handle.net/2440/117522
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dc.contributor.authorMaxted, N.I.en
dc.contributor.authorBraiding, C.en
dc.contributor.authorWong, G.F.en
dc.contributor.authorRowell, G.P.en
dc.contributor.authorBurton, M.G.en
dc.contributor.authorFilipović, M.D.en
dc.contributor.authorVoisin, F.en
dc.contributor.authorUrošević, D.en
dc.contributor.authorVukotić, B.en
dc.contributor.authorPavlović, M.Z.en
dc.contributor.authorSano, H.en
dc.contributor.authorFukui, Y.en
dc.date.issued2018en
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, 2018; 480(1):134-148en
dc.identifier.issn0035-8711en
dc.identifier.issn1365-2966en
dc.identifier.urihttp://hdl.handle.net/2440/117522-
dc.description.abstractThe Galactic supernova remnant HESSJ1534−571 (also known as G323.7 − 1.0) has a shell-like morphology in TeV gamma-ray emission and is a key object in the study of cosmic ray origin. Little is known about its distance and local environment. We examine Mopra 12CO/13CO(1–0) data, Australian Telescope Compact Array HI⁠, and Parkes HI data towards HESSJ1534−571⁠. We trace molecular clouds in at least five velocity ranges, including clumpy interstellar medium structures near a dip in HI emission at a kinematic velocity consistent with the Scutum–Crux arm at ∼3.5 kpc. This feature may be a cavity blown-out by the progenitor star, a scenario that suggests HESSJ1534−571 resulted from a core-collapse event. By employing parametrizations fitted to a sample of supernova remnants of known distance, we find that the radio continuum brightness of HESSJ1534−571 is consistent with the ∼3.5 kpc kinematic distance of the Scutum–Crux arm HI dip. Modelling of the supernova evolution suggests a ∼8–24 kyr age for HESSJ1534−571 at this distance.en
dc.description.statementofresponsibilityNigel I. Maxted, C. Braiding, G. F. Wong, G. P. Rowell ... Gavin P. Rowell ... Fabien Voisin ... et al.en
dc.language.isoenen
dc.publisherOxford University Pressen
dc.rights© 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Societyen
dc.subjectCosmic rays, ISM: molecules, ISM: supernova remnants, gamma-rays: ISMen
dc.titleSearching for an interstellar medium association for HESS J1534-571en
dc.typeJournal articleen
dc.identifier.rmid0030096856en
dc.identifier.doi10.1093/mnras/sty1797en
dc.relation.granthttp://purl.org/au-research/grants/arc/LE160100094en
dc.identifier.pubid435949-
pubs.library.collectionPhysics publicationsen
pubs.library.teamDS10en
pubs.verification-statusVerifieden
pubs.publication-statusPublisheden
dc.identifier.orcidRowell, G.P. [0000-0002-9516-1581]en
Appears in Collections:Physics publications

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