BVRH{alpha} photometry of candidates Be stars

DOI

We present B, V, R, and H{alpha} photometry of eight clusters in the Small Magellanic Cloud, five in the Large Magellanic Cloud, and three Galactic clusters and use two-color diagrams (2-CDs) to identify candidate Be star populations in these clusters. We find evidence that the Be phenomenon is enhanced in low-metallicity environments, based on the observed fractional early-type candidate Be star content of clusters of age 10-25Myr.

Cone search capability for table J/ApJ/652/458/table4 (Photometric properties of the candidate Be stars)

Identifier
DOI http://doi.org/10.26093/cds/vizier.16520458
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/ApJ/652/458
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/652/458
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/652/458
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/ApJ/652/458
Provenance
Creator Wisniewski J.P.; Bjorkman K.S.
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; Galactic and extragalactic Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy