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dc.contributor.authorGómez-Ruiz, AIen_US
dc.contributor.authorCodella, Cen_US
dc.contributor.authorViti, Sen_US
dc.contributor.authorJiménez-Serra, Ien_US
dc.contributor.authorNavarra, Gen_US
dc.contributor.authorBachiller, Ren_US
dc.contributor.authorCaselli, Pen_US
dc.contributor.authorFuente, Aen_US
dc.contributor.authorGusdorf, Aen_US
dc.contributor.authorLefloch, Ben_US
dc.contributor.authorLorenzani, Aen_US
dc.contributor.authorNisini, Ben_US
dc.date.accessioned2017-01-12T13:57:15Z
dc.date.available2016-07-21en_US
dc.date.issued2016-10-21en_US
dc.date.submitted2017-01-10T15:07:14.432Z
dc.identifier.issn1365-2966en_US
dc.identifier.urihttp://qmro.qmul.ac.uk/xmlui/handle/123456789/18509
dc.format.extent2203 - 2217en_US
dc.publisherOxford University Press (OUP)en_US
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen_US
dc.titleDiagnosing shock temperature with NH 3 and H 2 O profilesen_US
dc.typeArticle
dc.rights.holder© 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
dc.identifier.doi10.1093/mnras/stw1811en_US
pubs.issue2en_US
pubs.notesNot knownen_US
pubs.publication-statusPublisheden_US
pubs.volume462en_US
dcterms.dateAccepted2016-07-21en_US
qmul.funderMassive Star Formation with New Generation Interferometers::Science and Technology Facilities Council [2006-2012]en_US


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