Are infrared dark clouds really quiescent?-Reference-Cited by-同舟云学术

Are infrared dark clouds really quiescent?

Published:2016-07-06 Issue: Volume:592 Page:A21
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Feng S.,Beuther H.,Zhang Q.,Henning Th.,Linz H.,Ragan S.,Smith R.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361/201526864/pdf

Reference143 articles.

1. HCN in Bok Globules: A Good Tracer of Collapsing Cores

2. Molecular Evolution and Star Formation: From Prestellar Cores to Protostellar Cores

3. Fragmentation of elongated cylindrical clouds. I - Isothermal clouds

4. Bergin, E. A. 2003, in SFChem 2002: Chemistry as a Diagnostic of Star Formation, eds. C. L. Curry, & M. Fich (Ottawa: National Research Council Press), 63

5. Cold Dark Clouds: The Initial Conditions for Star Formation

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