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dc.contributor.authorViti, S.
dc.contributor.authorJones, H.R.A.
dc.contributor.authorRichter, M.J.
dc.contributor.authorBarber, R.J.
dc.contributor.authorTennyson, J.
dc.contributor.authorLacy, J.H.
dc.date.accessioned2009-01-05T09:36:20Z
dc.date.available2009-01-05T09:36:20Z
dc.date.issued2008
dc.identifier.citationViti , S , Jones , H R A , Richter , M J , Barber , R J , Tennyson , J & Lacy , J H 2008 , ' A potential new method for determining the temperature of cool stars ' , Monthly Notices of the Royal Astronomical Society , vol. 388 , no. 3 , pp. 1305-1313 . https://doi.org/10.1111/j.1365-2966.2008.13489.x
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 164226
dc.identifier.otherPURE UUID: 572556f5-5fd4-4814-b322-77b3fe4ba302
dc.identifier.otherdspace: 2299/2732
dc.identifier.otherScopus: 48049123700
dc.identifier.urihttp://hdl.handle.net/2299/2732
dc.description‘The definitive version is available at www.blackwell-synergy.com.’ Copyright Blackwell Publishing DOI: 10.1111/j.1365-2966.2008.13489.x
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.titleA potential new method for determining the temperature of cool starsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
rioxxterms.versionofrecordhttps://doi.org/10.1111/j.1365-2966.2008.13489.x
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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