Time-dependent star formation in OB associations

Details Time-dependent star formation in OB associations Time-dependent star formation in OB associations

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...290..185d&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 290, March 1, 1985, p. 185-190. Sponsorship: Fonds de la Recherche Fondamen

Astronomy and Astrophysics

Astrophysics

43

Main Sequence Stars, O Stars, Star Clusters, Star Formation, Stellar Mass, B Stars, Hertzsprung-Russell Diagram, Time Dependence

Scientific paper

The authors show that in the OB associations Per OB1 and Cen OB1, the
lower mass stars were formed first, the most massive stars being 10 -
20×106yr younger than the lower mass stars. It is shown
that this result cannot be due to selection effects. The consequences of
this time-dependent star formation are briefly discussed.

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