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dc.contributor.authorKarl, C.
dc.contributor.authorHeber, U.
dc.contributor.authorNapiwotzki, R.
dc.date.accessioned2008-01-30T10:37:02Z
dc.date.available2008-01-30T10:37:02Z
dc.date.issued2005
dc.identifier.citationKarl , C , Heber , U & Napiwotzki , R 2005 , Subdwarf B Binaries from the SPY Project . in In: Procs of the 14th European Workshop on White Dwarfs - ASP Conference Series 334 . Astronomical Society of the Pacific , pp. 369-374 .
dc.identifier.isbn1-58381-197-4
dc.identifier.isbn978-1-58381-268-6
dc.identifier.otherdspace: 2299/1448
dc.identifier.urihttp://hdl.handle.net/2299/1448
dc.descriptionOriginal paper can be found at: http://www.astrosociety.org/pubs/cs/328.html--Copyright Astronomical Society of the Pacific
dc.description.abstractIn the course of our search for double degenerate binaries as potential progenitors of type Ia supernovae with the ESO VLT (ESO - SN Ia progenitor survey - SPY), several sdB binaries were discovered. We report on the analysis of six radial velocity variable sdB stars from the SPY project. Radial velocity curves have been measured. Effective temperatures, surface gravities and helium abundances are determined, as well as metal abundances. We highlight some strong abundance anomalies.en
dc.format.extent368008
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofIn: Procs of the 14th European Workshop on White Dwarfs - ASP Conference Series 334
dc.titleSubdwarf B Binaries from the SPY Projecten
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 (CAR)
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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