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The Lynds 204 Complex: Magnetic Field Controlled Evolution?

Published online by Cambridge University Press:  04 August 2017

W.H. McCutcheon ,
F. J. Vrba ,
R. L. Dickman  and
D. P. Clemens
W.H. McCutcheon
Affiliation:
Department of Physics, University of British Columbia, Canada
F. J. Vrba
Affiliation:
U.S. Naval Observatory, Flagstaff, USA
R. L. Dickman
Affiliation:
Five College Radio Astronomy Observatory and Department of Physics and Astronomy, University of Massachusetts, USA
D. P. Clemens
Affiliation:
Five College Radio Astronomy Observatory and Department of Physics and Astronomy, University of Massachusetts, USA Steward Observatory, University of Arizona, USA Bart J. Bok Fellow 1985-1986

Extract

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The L204 dark cloud complex is a highly elongated structure stretching over 4 degrees in declination. Its total mass is 400 M⊙ with the more tenuous sections of the cloud being displaced in right ascension from the more heavily obscured parts.

Information

Type
I. Star Forming Processes in the Solar Neighborhood
Information
Symposium - International Astronomical Union , Volume 115: Star Forming Regions , 1987 , pp. 84 - 85
Copyright
Copyright © Reidel 1987