UVES/VLT spectra of white dwarfs

DOI

The ESO Supernova Ia Progenitor Survey (SPY) took high-resolution spectra of more than 1000 white dwarfs and pre-white dwarfs. About two thirds of the stars observed are hydrogen-dominated DA white dwarfs. Here we present a catalog and detailed spectroscopic analysis of the DA stars in the SPY. Atmospheric parameters effective temperature and surface gravity are determined for normal DAs. Double-degenerate binaries, DAs with magnetic fields or dM companions, are classified and discussed.

Cone search capability for table J/A+A/505/441/wd (All white dwarfs observed)

Identifier
DOI http://doi.org/10.26093/cds/vizier.35050441
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/505/441
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/505/441
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/505/441
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/505/441
Provenance
Creator Koester D.; Voss B.; Napiwotzki R.; Christlieb N.; Homeier D.; Lisker T.,Reimers D.; Heber U.
Publisher CDS
Publication Year 2010
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy