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
Antonio UribeObservatorio Astronómico Nacional, Facultad de Ciencias, Universidad Nacional de Colombia, Bogotá, Colombia;José‐Alejandro García‐VarelaObservatorio Astronómico Nacional, Facultad de Ciencias, Universidad Nacional de Colombia, Bogotá, Colombia;Beatriz‐Eugenia Sabogal‐MartínezObservatorio Astronómico Nacional, Facultad de Ciencias, Universidad Nacional de Colombia, Bogotá, Colombia;Mario A. Higuera G.Observatorio Astronómico Nacional, Facultad de Ciencias, Universidad Nacional de Colombia, Bogotá, Colombia;Eduardo BrievaObservatorio Astronómico Nacional, Facultad de Ciencias, Universidad Nacional de Colombia, Bogotá, Colombia;
2002en
ABI
Аннотация
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.
Ҳали таржима қилинмаган
Идентификаторлар
Иқтибослар ва манбалар
1 та иқтибос0 та фойдаланилган манба