Age subgroups in open clusters

Details Age subgroups in open clusters Age subgroups in open clusters

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...253..374s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 253, no. 2, Jan. 1992, p. 374-378.

Astronomy and Astrophysics

Astrophysics

10

Open Clusters, Star Distribution, Stellar Luminosity, Color-Magnitude Diagram, Stellar Evolution, Stellar Mass

Scientific paper

The analysis of the bright parts of the observed luminosity functions determined for 14 young clusters shows that most of these clusters consist of a few subgroups of different age. The sequentially-formed subgroups seem not to differ in their initial mass functions (IMF). The universal IMF resulting from the process of open cluster formation is similar to that of the field star determined by Scalo (1986).

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