Photometric Studies of Open Clusters: Be 95, Cze 21, Cze 38, Ju 11, King 17, and King 18

Details Photometric Studies of Open Clusters: Be 95, Cze 21, Cze 38, Ju 11, King 17, and King 18 Photometric Studies of Open Clusters: Be 95, Cze 21, Cze 38, Ju 11, King 17, and King 18

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aca....58..389m&link_type=abstract

Acta Astronomica, Vol. 58, p. 389

Astronomy and Astrophysics

Astronomy

3

Open Clusters And Associations: Individual: Berkeley 95, Czernik 21, Czernik 38, Jucher 11, King 17, King 18

Scientific paper

Results of investigations of six poorly studied or unstudied open clusters are presented. The ages, interstellar reddenings, distances, and structural parameters were derived based on BV photometry combined with the near-infrared JHKS data. The mass functions were analyzed for four objects and total masses, number of members, and dynamical-evolution parameters were estimated. Berkeley 95 was found to be an extremely young stellar cluster. King 17 and King 18 turned out to be an intermediate-age objects. Czernik 21, Czernik 38, and Juchert 11 were found to be old stellar ensembles of the age of about 1 Gyr old or older. Czernik 38 is located in the Sagittarius Arm while the remaining clusters belong to the Perseus Arm.

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