NGC 7142 Vilnius photometry

DOI

The results of medium-band photometry of 1037 stars in the area of the old open cluster NGC 7142 down to V=20.1mag in the Vilnius seven-colour system are presented. Photometric results are used to classify in spectral and luminosity classes about 80 per cent of stars down to V=18.5mag, to identify cluster members, to determine the main cluster parameters and to investigate the interstellar extinction in this direction. The average extinction A_V_ of the cluster is about 1.1mag [E(B-V)=0.35], and its distance is 2.3kpc (the distance modulus 11.8mag). The age of the cluster, 3.0Gyr, is estimated from the intrinsic colour-magnitude diagram with individual dereddening of each star and the Padova isochrones. The surface distribution of the extinction is shown. The reddening of the eclipsing variable V375 Cep is found to be close to the average reddening of the cluster. Probably, the cluster contains five red clump giants, two asymptotic branch stars and four blue stragglers.

Cone search capability for table J/MNRAS/437/1628/table2 (Results of photometry and classification of stars in the NGC 7142 area measured in the Vilnius 7-colour system)

Identifier
DOI http://doi.org/10.26093/cds/vizier.74371628
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/437/1628
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/437/1628
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/437/1628
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/MNRAS/437/1628
Provenance
Creator Straizys V.; Maskoliunas M.; Boyle R.P.; Zdanavicius K.; Zdanavicius J.,Laugalys V.; Kazlauskas A.
Publisher CDS
Publication Year 2015
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