Physical parameters of the DA white dwarfs from ESO SN Ia Progenitor Survey data

Details Physical parameters of the DA white dwarfs from ESO SN Ia Progenitor Survey data Physical parameters of the DA white dwarfs from ESO SN Ia Progenitor Survey data

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1273...44n&link_type=abstract

17TH EUROPEAN WHITE DWARF WORKSHOP. AIP Conference Proceedings, Volume 1273, pp. 44-47 (2010).

Computer Science

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White Dwarfs, Sky Surveys, Brightness, Bolometers, Faint Blue Stars, White Dwarfs, Degenerate Stars, Nuclei Of Planetary Nebulae, Astronomical Catalogs, Atlases, Sky Surveys, Databases, Retrieval Systems, Archives, Etc., Luminosity And Mass Functions, Photoconductors And Bolometers

Scientific paper

We present determinations of masses, radii and bolometric luminosities for DA white dwarfs observed for the ESO SN Ia Progenitor Survey. Masses and radii of 513 stars were determined from their effective temperatures and surface gravities, obtained by Koester et al. (2009 [6]). We have used a grid of theoretical mass-radius relations for carbon and oxygen core stars with hydrogen envelopes derived by Panei et al. (2000 [10]).

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