Photometric Evolution of Open Clusters and Associations

Details Photometric Evolution of Open Clusters and Associations Photometric Evolution of Open Clusters and Associations

Apr 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993jkas...26...47l&link_type=abstract

Journal of the Korean Astronomical Society, vol. 26, no. 1, p. 47-64

Astronomy and Astrophysics

Astronomy

1

Open Clusters, Associations

Scientific paper

The photometric evolution of cluster stars are examined for six synthetic clusters in the age range from 2.4*10E6 yr to 7.6*10E8 yr by using the detailed evolutionary model calculation, and their results are compared with the observed integrated absolute magnitude and colors of 47 clusters. The reasonable agreements of the observed photometric parameters with the synthetic evolutionary sequences imply that there is a general form of time-dependent IMF including the noncoeval formation of stars and its detailed function is changed slightly with various environmental conditions of each primordial cloud.

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