Photometry of DE CVn

DOI

Close white dwarf-red dwarf binaries must have gone through a common-envelope phase during their evolution. DE CVn is a detached white dwarf-red dwarf binary with a relatively short (~8.7h) orbital period. Its brightness and the presence of eclipses makes this system ideal for a more detailed study. From a study of photometric and spectroscopic observations of DE CVn we derive the system parameters that we discuss in the framework of common-envelope evolution.

Identifier
DOI http://doi.org/10.26093/cds/vizier.34661031
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/466/1031
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/466/1031
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/466/1031
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/466/1031
Provenance
Creator van den Besselaar E.J.M.; Greimel R.; Morales-Rueda L.; Nelemans G.,Thorstensen R.; Marsh T.R.; Dhillon V.S.; Robb R.M.; Balam D.D.,Guenther E.W.; Kemp J.; Augusteijn T.; Groot P.J.
Publisher CDS
Publication Year 2007
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