uvby{beta} photometry of h and chi Per

DOI

We present CCD uvby{beta} photometry for stars in the nuclei of the young double cluster {h} and {chi} Persei. We find that the reddening is highly variable through the {h} Per nucleus, increasing from west to east, with values ranging from E(b-y)=0.328+/-0.022 in the western part to E(b-y)=0.465+/-0.025 in the south-east. Towards {chi} Persei the reddening is fairly constant, with E(b-y)=0.398+/-0.025. Both clusters share a common distance modulus of 11.7+/-0.1mag, and an age of logt=7.10+/-0.05 years.

Cone search capability for table J/A+A/394/479/table6 (Coordinates and photometry for stars in h Per)

Cone search capability for table J/A+A/394/479/table7 (Coordinates and photometry for stars in chi Per)

Identifier
DOI http://doi.org/10.26093/cds/vizier.33940479
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/394/479
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/394/479
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/394/479
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/394/479
Provenance
Creator Capilla; G.; Fabregat J.
Publisher CDS
Publication Year 2003
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