h and {chi} Per memberships Virtual Observatory Resource

Authors

1. Uribe A.
2. Garcia-Varela J.-A.
3. Sabogal-Martinez B.-E.
4. Higuera G.M.A.,Brieva E.

Published by

CDS

Abstract

A segregation between cluster members and field stars in the region of the double cluster h and {chi} Persei is accomplished working from proper motions and positions as kinematic random variables. The extinction R_V_ and the distance moduli are determined once the physical cluster members are found.

Keywords

1. open-star-clusters
2. proper-motions

Bibliographic source Bibcode

2002PASP..114..233U

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/PASP/114/233

IVOA Identifier IVOID

ivo://CDS.VizieR/J/PASP/114/233

Access

Web browser access HTML

https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/PASP/114/233
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/PASP/114/233
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/PASP/114/233

IVOA Table Access TAP

https://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

IVOA Cone Search SCS

For use with a cone search client (e.g., TOPCAT).
https://vizier.cds.unistra.fr/viz-bin/conesearch/J/PASP/114/233/table2?
https://vizier.iucaa.in/viz-bin/conesearch/J/PASP/114/233/table2?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/PASP/114/233/table2?