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2002PASP..114..233U - Publ. Astron. Soc. Pac., 114, 233-248 (2002/February-0)

Membership in the region of the double cluster h and χ Persei working from proper motions and positions: distance moduli and extinction in that galactic direction.

URIBE A., GARCIA-VARELA J.-A., SABOGAL-MARTINEZ B.-E., HIGUERA G.M.A. and BRIEVA E.

Abstract (from CDS):

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.

Abstract Copyright:

Journal keyword(s): open clusters and associations: individual (χ Persei) - open clusters and associations: individual (h Persei) - ISM: Dust, Extinction - Methods: Data Analysis - Stars: Distances - Stars: Hertzsprung-Russell Diagram - Galaxy: Open Clusters and Associations: General

VizieR on-line data: <Available at CDS (J/PASP/114/233): table2.dat>

Simbad objects: 757

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