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Physical conditions of star forming sites in the S247/252 molecular complex

Published online by Cambridge University Press:  03 August 2017

C. Koempe ,
G. Joncas ,
J.G.A. Wouterloot  and
H. Meyerdierks
C. Koempe
Affiliation:
IRAM, Granada, Spain Max—Planck—Institut für Radioastronomie, Bonn, Fed. Rep. of Germany
G. Joncas
Affiliation:
Dépt. de Physique, Université Laval, Qu ébec, Canada
J.G.A. Wouterloot
Affiliation:
I. Physikalisches Institut, Universität zu Köln, Köln, Fed. Rep. of Germany
H. Meyerdierks
Affiliation:
Radioastronomisches Institut, Universität Bonn, Bonn, Fed. Rep. of Germany

Extract

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By now, it is well established that massive stars form in giant molecular clouds. Numerous studies have shown that star formation, instead of being spread uniformly throughout molecular clouds, occurs in dense condensations located within these clouds. The physical conditions in these condensations are therefore critical input parameters for any theory of star formation.

Type
Poster Sessions
Information
Symposium - International Astronomical Union , Volume 147: Fragmentation of Molecular Clouds and Star Formation , 1991 , pp. 443 - 444
Copyright
Copyright © Kluwer 1991 

References

Koempe, C., Joncas, G., Baudry, A., Wouterloot, J.G.A., Astron. Astrophys., 221, (1989)Google Scholar
Lada, C.L., Wooden, D., Astrophys. J., 232, 158, (1979)Google Scholar