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dc.contributor.authorEdelmann, H.
dc.contributor.authorHeber, U.
dc.contributor.authorNapiwotzki, R.
dc.contributor.authorReid, I.N.
dc.contributor.authorSaffer, R.
dc.date.accessioned2008-01-27T15:29:47Z
dc.date.available2008-01-27T15:29:47Z
dc.date.issued1999
dc.identifier.citationEdelmann , H , Heber , U , Napiwotzki , R , Reid , I N & Saffer , R 1999 , Spectral analysis of the binary sdB star Feige 36 . in In: Procs of the 11th European Workshop on White Dwarfs, ASP Conference Series 169 . Astronomical Society of the Pacific , pp. 546-550 .
dc.identifier.isbn1-886733-91-0
dc.identifier.otherPURE: 142971
dc.identifier.otherPURE UUID: 98a48ed6-1aa7-43b7-85ff-1ad5a256a461
dc.identifier.otherdspace: 2299/1422
dc.identifier.urihttp://hdl.handle.net/2299/1422
dc.descriptionOriginal paper can be found at: http://www.astrosociety.org/pubs/cs/156-194.html--Copyright Astronomical Society of the Pacific
dc.description.abstractThe sdB stars Feige 36 is a short-period, single-lined spectroscopic binary. Aymospheric parameters and abundances are determined from high-resolution Keck spectra. Feige 36 lies near the zero-age extreme Horizontal Branch position in the HRD.en
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofIn: Procs of the 11th European Workshop on White Dwarfs, ASP Conference Series 169
dc.rightsOpen
dc.titleSpectral analysis of the binary sdB star Feige 36en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dcterms.dateAccepted1999
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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