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dc.contributor.authorKoester, D.
dc.contributor.authorRollenhagen, K.
dc.contributor.authorNapiwotzki, R.
dc.contributor.authorVoss, B.
dc.contributor.authorChristlieb, N.
dc.contributor.authorHomeier, D.
dc.contributor.authorReimers, D.
dc.date.accessioned2008-01-30T10:37:00Z
dc.date.available2008-01-30T10:37:00Z
dc.date.issued2005
dc.identifier.citationKoester , D , Rollenhagen , K , Napiwotzki , R , Voss , B , Christlieb , N , Homeier , D & Reimers , D 2005 , DAZ White Dwarfs in the SPY Sample . in In: Procs of the 14TH European Workshop on White Dwarfs - ASP Conference Series 334 . Astronomical Society of the Pacific , pp. 215-220 .
dc.identifier.isbn1-58381-197-4
dc.identifier.isbn978-1-58381-268-6
dc.identifier.otherPURE: 144843
dc.identifier.otherPURE UUID: 28bf91f5-f210-42a1-bab3-fb5e45193fa3
dc.identifier.otherdspace: 2299/1444
dc.identifier.urihttp://hdl.handle.net/2299/1444
dc.descriptionOriginal paper can be found at: http://www.astrosociety.org/pubs/cs/328.html--Copyright Astronomical Society of the Pacific
dc.description.abstractWe search for faint Ca II lines in the spectra of about 800 apparently single white dwarfs observed at high resolution for the SPY (ESO Supernova Progenitor Survey) survey. Photospheric Ca is detected in 24 DAZ; in 25 mostly hot objects the observed lines must be interstellar. The distribution of metal abundances is discussed and compared with the predictions of the accretion/ diffusion scenario. We argue that the observations are easier to understand in a scenario of continuous ongoing accretion with rates varying with the conditions of the ambient medium, rather than with the strongly idealized \two phase accretion/diffusion scenario" of Dupuis et al. (1992, 1993a, 1993b).en
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.titleDAZ White Dwarfs in the SPY Sampleen
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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