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dc.contributor.authorHindson, Luke
dc.contributor.authorThompson, Mark
dc.contributor.authorUrquhart, J.S.
dc.contributor.authorFaimali, Alessandro
dc.contributor.authorJohnston-Hollitt, M.
dc.contributor.authorClark, J. S.
dc.contributor.authorDavies, B.
dc.date.accessioned2014-08-20T11:30:45Z
dc.date.available2014-08-20T11:30:45Z
dc.date.issued2013-11-01
dc.identifier.citationHindson , L , Thompson , M , Urquhart , J S , Faimali , A , Johnston-Hollitt , M , Clark , J S & Davies , B 2013 , ' The G305 star-forming complex : radio continuum and molecular line observations ' , Monthly Notices of the Royal Astronomical Society , vol. 435 , no. 3 , pp. 2003-2022 . https://doi.org/10.1093/mnras/stt1405
dc.identifier.issn0035-8711
dc.identifier.otherORCID: /0000-0001-5392-909X/work/30970784
dc.identifier.urihttp://hdl.handle.net/2299/14398
dc.description.abstractWe present 109–115 GHz (3 mm) wide-field spectral line observations of 12CO, 13CO and C18O J = 1–0 molecular emission and 5.5 and 8.8 GHz (6 and 3 cm) radio continuum emission towards the high-mass star-forming complex known as G305. The morphology of G305 is dominated by a large evacuated cavity at the centre of the complex driven by clusters of O stars surrounded by molecular gas. Our goals are to determine the physical properties of the molecular environment and reveal the relationship between the molecular and ionized gas and star formation in G305en
dc.format.extent13000784
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.titleThe G305 star-forming complex : radio continuum and molecular line observationsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research (CAR)
dc.description.statusPeer reviewed
rioxxterms.versionofrecord10.1093/mnras/stt1405
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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