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Star formation in three nearby cloud complexes

Published online by Cambridge University Press:  03 August 2017

Neal J. Evans II  and
Elizabeth A. Lada
Neal J. Evans II
Affiliation:
Astronomy Department, The University of Texas, Austin Texas 78712, USA E-mail NJE@ASTRO.AS.UTEXAS.EDU
Elizabeth A. Lada
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA E-mail LADA@CFA.BITNET

Abstract

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We consider the distribution and nature of the gas and star formation in three nearby molecular cloud complexes: Taurus-Auriga, Ophiuchus, and Orion. Large-scale studies show that quite different distributions of dense gas and star formation exist in these regions, but that the global efficiency of star formation, so far, is about 1% in all of these complexes, very similar to the final efficiencies deduced for open clusters and associations. Furthermore, evidence for differences in the initial mass function among these regions is weak; all three regions may be compatible with the initial mass function for open clusters and field stars. Finally, we consider specific examples of star formation in each complex; the results indicate that the ideas of Adams, Lada, and Shu (1987) are reasonably consistent with the data on L1551 IRS 5, in the Taurus cloud, but that modifications are likely to be needed for IRAS 16293-2422 in Ophiuchus and for NGC2071 in Orion.

Keywords

star formationmolecular cloudsembedded clusters
Type
Star Formation
Information
Symposium - International Astronomical Union , Volume 147: Fragmentation of Molecular Clouds and Star Formation , 1991 , pp. 293 - 315
Copyright
Copyright © Kluwer 1991 

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