BV(RI)c light curves of BS Com

We derive the basic physical parameters of the field double-mode RR Lyrae star BS Com from its observed periods and the requirement of consistency between the pulsational and evolutionary constraints. We performed a standard frequency analysis on the V data by discrete Fourier transformation. We derived P0=0.48791d and P1=0.36307d for the periods of the fundamental and the first overtone modes, respectively.

Identifier
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/386/521
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/386/521
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/386/521
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/MNRAS/386/521
Provenance
Creator Dekany I.; Kovacs G.; Jurcsik J.; Szabo R.; Varadi M.; Sodor A.,Posztobanyi K.; Hurta Zs.; Vida K.; Vityi N.; Szing A.
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