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dc.contributor.authorDrilling, J.S.en_US
dc.contributor.authorNapiwotzki, R.en_US
dc.contributor.authorDreizler, S.en_US
dc.contributor.authorHeber, U.en_US
dc.contributor.authorBeers, T.C.en_US
dc.date.accessioned2008-01-27T15:29:46Z
dc.date.available2008-01-27T15:29:46Z
dc.date.issued1996en_US
dc.identifier.citationIn: Hydrogen deficient stars, ASP Conference Series 96 p.317en_US
dc.identifier.isbn1-886733-17-1en
dc.identifier.other901585en_US
dc.identifier.urihttp://hdl.handle.net/2299/1419
dc.descriptionOriginal paper can be found at: http://www.astrosociety.org/pubs/cs/070-112.html--Copyright Astronomical Society of the Pacificen
dc.description.abstractWe have determined effective temperatures, surface gravities, and helium-to-hydrogen abundance ratios by fitting NLTE model atmospheres to high signal-to-noise- spectra of eight helium-rich sdO stars detected in the southern HK survey.en
dc.format.extent53426 bytes
dc.format.mimetypeapplication/pdf
dc.language.isoen_US
dc.publisherAstronomical Society of the Pacificen_US
dc.titleNLTE spectral analysis of helium-rich sdO stars from the southern HK survey.en_US
dc.typeConference paperen_US
herts.preservation.rarelyaccessedtrue


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