The initial mass function of the Coma Berenices open cluster (MEL 111)

Details The initial mass function of the Coma Berenices open cluster (MEL 111) The initial mass function of the Coma Berenices open cluster (MEL 111)

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...260..112b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 260, no. 1-2, p. 112-114.

Astronomy and Astrophysics

Astrophysics

5

Hertzsprung-Russell Diagram, Open Clusters, Stellar Mass, Radial Velocity, Star Distribution

Scientific paper

The HR (log T(eff), M(bol)) diagram of the Coma Berenices open cluster (MEL 111), as derived from a reliable list of cluster members, is employed to show that its IMF can be approximated by a power law of stellar mass with a slope of x = 1.90 in the mass range 1-2.5 solar masses. The HR diagram of the Coma Berenices open cluster, and star counts of Coma Berenices are presented.

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