h and χ Per memberships (Uribe+, 2002)

Details h and χ Per memberships (Uribe+, 2002) h and χ Per memberships (Uribe+, 2002)

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ycat..61140233u&link_type=abstract

VizieR On-line Data Catalog: J/PASP/114/233. Originally published in: 2002PASP..114..233U

Physics

Clusters: Open, Proper Motions

Scientific paper

A segregation between cluster members and field stars in the region of the double cluster h and χ Persei is accomplished working from proper motions and positions as kinematic random variables. The extinction RV and the distance moduli are determined once the physical cluster members are found.
(1 data file).

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