UBV Photometry in NGC 7419

DOI

UBV CCD photometry has been carried out on the heavily reddened (A_V_=6.7) Cepheus open cluster NGC 7419. An age of 14+/-2 Myr and a distance of 2.3kpc have been derived using the isochrones of Maeder. The mass function of the cluster satisfies the Salpeter from n(M)~M^-{gamma}^ with {gamma}=2.25. The cluster is dynamically relaxed.

Cone search capability for table J/ApJS/93/187/table1 (Coordinates and mean magnitudes of the 518 stars in NGC 7419 with measured V and B magnitudes)

Identifier
DOI http://doi.org/10.26093/cds/vizier.20930187
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/ApJS/93/187
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/93/187
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/93/187
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/ApJS/93/187
Provenance
Creator Beauchamp A.; Moffat A.F.J.; Drissen L.
Publisher CDS
Publication Year 2009
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