Clouds as Turbulent Density Fluctuations: Implications for Pressure Confinement and Spectral Line Data Interpretation-Reference-Cited by-同舟云学术

Clouds as Turbulent Density Fluctuations: Implications for Pressure Confinement and Spectral Line Data Interpretation

Published:1999-04-10 Issue:1 Volume:515 Page:286-303
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Ballesteros‐Paredes Javier,Vazquez‐Semadeni Enrique,Scalo John

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/515/i=1/a=286/pdf

Reference106 articles.

1. Ambiguities in the identification of giant molecular cloud complexes from longitude-velocity diagrams

2. Alves, J., Lada, C. & Lada, E. 1999, ApJ, in press

3. A detailed examination of the kinematics of rotating dark clouds

4. Ballesteros-Paredes, J. & Vazquez-Semadeni, E. 1995, in Proc. Rev. Mexicana Astron. Astrofis. Conf. Ser. 3, Fifth Mexico-Texas Conference on Astrophysics, ed. M. Pena & S. Kurtz, 105

5. Ballesteros-Paredes, J. & Vazquez-Semadeni, E. 1999, in preparation

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