Simulating star formation in molecular cloud cores-Reference-Cited by-同舟云学术

Simulating star formation in molecular cloud cores

Published:2009-01-14 Issue:1 Volume:495 Page:201-215
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Attwood R. E.,Goodwin S. P.,Stamatellos D.,Whitworth A. P.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361:200810806/pdf

Reference72 articles.

1. Internal structure of a cold dark molecular cloud inferred from the extinction of background starlight

2. The mass function of dense molecular cores and the origin of the IMF

3. André, P., Ward-Thompson, D., & Barsony, M. 2000, Protostars & Planets IV ed. V. Mannings, A. P. Boss, & S. S. Russell (Tucson: Univ. of Arizona Press), 59

4. The initial conditions of star formation in the Ophiuchus main cloud: Kinematics of the protocluster condensations

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