V505 Per BV light curves

DOI

The orbit and fundamental physical parameters of the double-lined eclipsing binary V505 Per are derived by means of Echelle high-resolution and high S/N spectroscopy, and B, V photometry. In addition, effective temperatures, gravities, rotational velocities, and metallicities of both components are also obtained from atmospheric chi^2^ analysis, showing an excellent match with the results of the orbital solution.

Identifier
DOI http://doi.org/10.26093/cds/vizier.34800465
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/480/465
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/480/465
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/480/465
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/480/465
Provenance
Creator Tomasella L.; Munari U.; Siviero A.; Cassisi S.; Dallaporta S.; Zwitter T.,Sordo R.
Publisher CDS
Publication Year 2008
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