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dc.contributor.authorVoss, B.
dc.contributor.authorKoester, D.
dc.contributor.authorOstensen, R.
dc.contributor.authorNapiwotzki, R.
dc.contributor.authorHomeier, D.
dc.contributor.authorReimers, D.
dc.date.accessioned2008-06-27T14:13:06Z
dc.date.available2008-06-27T14:13:06Z
dc.date.issued2007
dc.identifier.citationVoss , B , Koester , D , Ostensen , R , Napiwotzki , R , Homeier , D & Reimers , D 2007 , Six New ZZ Ceti Stars from the SPY and the HQS Surveys . in In: Procs of the 15th European Workshop on White Dwarfs - ASP Conf Series 372 . Astronomical Society of the Pacific , pp. 583-586 .
dc.identifier.isbn978-1-58381-239-6
dc.identifier.isbn978-1-58381-306-5
dc.identifier.otherdspace: 2299/2146
dc.identifier.urihttp://hdl.handle.net/2299/2146
dc.descriptionOriginal paper can be found at: http://www.astrosociety.org/pubs/cs/361.html Copyright ASP
dc.description.abstractWe report on the discovery of six new ZZCeti stars. They were selected as candidates based on preparatory photometric observations of ob- jects from the Hamburg Quasar Survey (HQS), and based on the spectra of the Supernova Ia Progenitor Survey (SPY). Time-series photometry of 19 can- didate stars was carried out at the Nordic Optical Telescope (NOT) at Roque de Los Muchachos Observatory, Spain. The new variables are relatively bright, 15.4 < B < 16.6. Among them is WD 1150−153, which is the third ZZCeti star that shows photospheric CaII in its spectrum.en
dc.format.extent195608
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofIn: Procs of the 15th European Workshop on White Dwarfs - ASP Conf Series 372
dc.titleSix New ZZ Ceti Stars from the SPY and the HQS Surveysen
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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