UBV(RI)c photometry of 4 open clusters

DOI

Ages derived from the low mass stars still contracting onto the main sequence often differ from ages derived from the high mass ones that have already evolved away from it. We investigate the general claim of disagreement between these two independent age determinations by representing UBVRI photometry of the young galactic open clusters NGC 2232, NGC 2516, NGC 2547 and NGC 4755, spanning the age range ~10-150Myr.

Cone search capability for table J/A+A/453/101/phot (Photometry in 4 clusters NGC 2232, NGC 2516, NGC 2547 and NGC 4755 (tables 6-9 of paper))

Identifier
DOI http://doi.org/10.26093/cds/vizier.34530101
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/453/101
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/453/101
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/453/101
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/453/101
Provenance
Creator Lyra W.; Moitinho A.; van der Bliek N.S.; Alves J.F.
Publisher CDS
Publication Year 2019
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