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dc.contributor.authorJones, H.R.A.
dc.contributor.authorLongmore, A.J.
dc.contributor.authorJameson, R.F.
dc.date.accessioned2008-02-01T11:43:59Z
dc.date.available2008-02-01T11:43:59Z
dc.date.issued1994
dc.identifier.citationJones , H R A , Longmore , A J & Jameson , R F 1994 , An Infrared Spectral Sequence for M Dwarfs . in In: Cool Stars, Stellar Systems and the Sun; Eighth Cambridge Workshop - ASP Conf Series 64 . Astronomical Society of the Pacific , pp. 614-8 .
dc.identifier.isbn0-937707-83-X
dc.identifier.otherPURE: 142559
dc.identifier.otherPURE UUID: 6eb79fbe-ba3a-4597-b764-4d2b7c4610a0
dc.identifier.otherdspace: 2299/1529
dc.identifier.urihttp://hdl.handle.net/2299/1529
dc.descriptionOriginal paper can be found at: http://www.astrosociety.org/pubs/cs/035-069.html--Copyright Astronomical Society of the Pacific
dc.description.abstractWe present a spectral sequence from 1-2.5 um of M dwarfs from GL411 which is classified as M2V to the best brown dwarf candidate GD165B (M10V). This sequence shows the progressive importance of water vapour in the stmospheres of M dwarfs. We take the strength of the water absorption bands as the basis of a new method to derive effective temperatures. We also identify many of the stronger atomic and molecular features and find that their strengths correlate with our derived temperature scale.en
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofIn: Cool Stars, Stellar Systems and the Sun; Eighth Cambridge Workshop - ASP Conf Series 64
dc.rightsOpen
dc.titleAn Infrared Spectral Sequence for M Dwarfsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dcterms.dateAccepted1994
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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