Hostname: page-component-848d4c4894-ttngx Total loading time: 0 Render date: 2024-05-27T04:34:24.477Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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.

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