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dc.contributor.authorHindson, Luke
dc.contributor.authorNapiwotzki, R.
dc.contributor.authorHeber, U.
dc.contributor.authorLemke, M.
dc.date.accessioned2008-10-03T10:28:29Z
dc.date.available2008-10-03T10:28:29Z
dc.date.issued2008
dc.identifier.citationHindson , L , Napiwotzki , R , Heber , U & Lemke , M 2008 , Model Spectra of Hot Subdwarfs for the Gaia Mission . in In: Hot Subdwarf Stars and Related Objects - ASP Conference Series 392 . Astronomical Society of the Pacific , pp. 163-166 .
dc.identifier.isbn978-1-58381-654-7
dc.identifier.isbn978-1-58381-655-4
dc.identifier.otherPURE: 168085
dc.identifier.otherPURE UUID: afaf26d5-c642-4487-91c7-f1c37121b87c
dc.identifier.otherdspace: 2299/2428
dc.identifier.urihttp://hdl.handle.net/2299/2428
dc.descriptionOriginal paper can be found at: http://astrosociety.org/pubs/cs/381.html Copyright ASP
dc.description.abstractThe Gaia mission will provide an unprecedented 3D view of our galaxy, it will obtain astrometric, photometric and spectrographic data for roughly one billion stars. We are particularly interested in the treasure chest of new data Gaia will produce for hot subdwarf B (sdB) stars. In order for Gaia to classify sdBs and estimate parameters model spectra covering a wide parameter range are needed. Here we describe the construction of an extensive grid, which will be used for this purpose.en
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofIn: Hot Subdwarf Stars and Related Objects - ASP Conference Series 392
dc.titleModel Spectra of Hot Subdwarfs for the Gaia Missionen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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