High Velocity CO Line Wings and the Dynamics of Star Forming Molecular Cloud Cores-Reference-Cited by-同舟云学术

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High Velocity CO Line Wings and the Dynamics of Star Forming Molecular Cloud Cores

Published:1982 Issue: Volume: Page:287-293
ISSN:0067-0057
Container-title:Regions of Recent Star Formation
language:
Short-container-title:

Author:

Bally John

Publisher

Springer Netherlands

Link

http://link.springer.com/content/pdf/10.1007/978-94-009-7778-5_37

Reference12 articles.

1. Bally3 J. (1981) Ap J (submitted).

2. Bally, J. and Predmore, R. (1981) Ap J (in preparation).

3. Harvey, P. M., Campbell, M. F., Hoffman, W. F., Thronsen, H.A. and Gatley, I. (1979) Ap J 229, 990.

4. Snell, R. L. and Edwards, S. (1982) this volume, p. 173.

5. Lada, C. J. (1981) private communication.

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1. The Distribution of Thermal Pressures in the Interstellar Medium from a Survey of C i Fine‐Structure Excitation;The Astrophysical Journal Supplement Series;2001-12

2. The Properties of Molecular Hydrogen toward the Orion Belt Stars from Observations by the Interstellar Medium Absorption Profile Spectrograph;The Astrophysical Journal;2000-07-20

3. A Catalogue of Extremely Young, Massive and Compact Infrared Objects (Mitteilungen der Universitäts-Sternwarte zu Jena Nr. 165);Astronomische Nachrichten: A Journal on all Fields of Astronomy;1984-01-27

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