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dc.contributor.authorJones, H.R.A.
dc.contributor.authorTsuji, Takashi
dc.date.accessioned2012-01-17T18:01:09Z
dc.date.available2012-01-17T18:01:09Z
dc.date.issued1997-02-13
dc.identifier.citationJones , H R A & Tsuji , T 1997 , ' Spectral evidence for dust in late-type M dwarfs ' , Astrophysical Journal Letters , vol. 480 , L39 . https://doi.org/10.1086/310619
dc.identifier.issn2041-8213
dc.identifier.otherPURE: 526396
dc.identifier.otherPURE UUID: 1c20050a-4c2a-4340-83a5-7b62b165ff95
dc.identifier.otherArXiv: http://arxiv.org/abs/astro-ph/9702108v1
dc.identifier.otherScopus: 21744442831
dc.identifier.urihttp://hdl.handle.net/2299/7676
dc.description9 pages, 5 postscript figs, ApJL accepted
dc.description.abstractWe have found a dramatic change in the spectra of late-type M dwarfs at wavelengths shorter than 0.75 microns. Comparisons with synthetic spectra illustrate that this change is well explained by the presence of dust. It thus seems that a substantial part of the long-standing discrepancies between late-type M dwarf models and observations arises from dust as recently proposed by Tsuji, Ohnaka and Aoki (1996a).en
dc.language.isoeng
dc.relation.ispartofAstrophysical Journal Letters
dc.rights/dk/atira/pure/core/openaccesspermission/open
dc.subjectastro-ph
dc.titleSpectral evidence for dust in late-type M dwarfsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dc.description.versiontypeSubmitted Version
rioxxterms.versionSMUR
rioxxterms.versionofrecordhttps://doi.org/10.1086/310619
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstyperestrictedAccess


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