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dc.contributor.authorHindson, L.
dc.contributor.authorJohnston-Hollitt, M.
dc.contributor.authorHurley-Walker, N.
dc.contributor.authorCallingham, J. R.
dc.contributor.authorSu, H.
dc.contributor.authorMorgan, J.
dc.contributor.authorBell, M.
dc.contributor.authorBernardi, G.
dc.contributor.authorBowman, J. D.
dc.contributor.authorBriggs, F.
dc.contributor.authorCappallo, R. J.
dc.contributor.authorDeshpande, A. A.
dc.contributor.authorDwarakanath, K. S.
dc.contributor.authorFor, B. -Q
dc.contributor.authorGaensler, B. M.
dc.contributor.authorGreenhill, L. J.
dc.contributor.authorHancock, P.
dc.contributor.authorHazelton, B. J.
dc.contributor.authorKapinska, A. D.
dc.contributor.authorKaplan, D. L.
dc.contributor.authorLenc, E.
dc.contributor.authorLonsdale, C. J.
dc.contributor.authorMckinley, B.
dc.contributor.authorMcWhirter, S. R.
dc.contributor.authorMitchell, D. A.
dc.contributor.authorMorales, M. F.
dc.contributor.authorMorgan, E.
dc.contributor.authorOberoi, D.
dc.contributor.authorOffringa, A.
dc.contributor.authorOrd, S. M.
dc.contributor.authorProcopio, P.
dc.contributor.authorPrabu, T.
dc.contributor.authorUdayaShankar, N.
dc.contributor.authorSrivani, K. S.
dc.contributor.authorStaveley-Smith, L.
dc.contributor.authorSubrahmanyan, R.
dc.contributor.authorTingay, S. J.
dc.contributor.authorWayth, R. B.
dc.contributor.authorWebster, R. L.
dc.contributor.authorWilliams, A.
dc.contributor.authorWilliams, C. L.
dc.contributor.authorWu, C.
dc.contributor.authorZheng, Q.
dc.date.accessioned2017-06-26T15:20:51Z
dc.date.available2017-06-26T15:20:51Z
dc.date.issued2016-05-17
dc.identifier.citationHindson , L , Johnston-Hollitt , M , Hurley-Walker , N , Callingham , J R , Su , H , Morgan , J , Bell , M , Bernardi , G , Bowman , J D , Briggs , F , Cappallo , R J , Deshpande , A A , Dwarakanath , K S , For , B -Q , Gaensler , B M , Greenhill , L J , Hancock , P , Hazelton , B J , Kapinska , A D , Kaplan , D L , Lenc , E , Lonsdale , C J , Mckinley , B , McWhirter , S R , Mitchell , D A , Morales , M F , Morgan , E , Oberoi , D , Offringa , A , Ord , S M , Procopio , P , Prabu , T , UdayaShankar , N , Srivani , K S , Staveley-Smith , L , Subrahmanyan , R , Tingay , S J , Wayth , R B , Webster , R L , Williams , A , Williams , C L , Wu , C & Zheng , Q 2016 , ' A Large Scale, Low Frequency Murchison Widefield Array Survey of Galactic HII regions between 260\340 ' , Publications of the Astronomical Society of Australia , vol. 33 , e020 . https://doi.org/10.1017/pasa.2016.19
dc.identifier.issn1323-3580
dc.identifier.otherArXiv: http://arxiv.org/abs/1605.02872v2
dc.identifier.urihttp://hdl.handle.net/2299/18532
dc.descriptionPublications of the Astronomical Society of Australia (PASA), Vol. 33, e020, 17 pages (2016). © Astronomical Society of Australia 2016; published by Cambridge University Press. The online version of this article is published within an Open Access environment subject to the conditions of the Creative Commons Attribution-NonCommercial-ShareAlike license http://creativecommons.org/licenses/ by-nc-sa/3.0/. The written permission of Cambridge University Press must be obtained for commercial re-use. doi:10.1017/pasa.2016.19
dc.description.abstractWe have compiled a catalogue of HII regions detected with the Murchison Widefield Array (MWA) between 72 and 231MHz. The multiple frequency bands provided by the MWA allow us identify the characteristic spectrum generated by the thermal Bremsstrahlung process in HII regions. We detect 302 HII regions between 260en
dc.format.extent1458319
dc.language.isoeng
dc.relation.ispartofPublications of the Astronomical Society of Australia
dc.subjectastro-ph.GA
dc.titleA Large Scale, Low Frequency Murchison Widefield Array Survey of Galactic HII regions between 260\340en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
rioxxterms.versionofrecord10.1017/pasa.2016.19
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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