On the role of the H2ortho:para ratio in gravitational collapse during star formation-Reference-Cited by-同舟云学术

On the role of the H2ortho:para ratio in gravitational collapse during star formation

Published:2014-03 Issue: Volume:563 Page:A85
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Vaytet Neil,Tomida Kengo,Chabrier Gilles

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361/201322855/pdf

Reference46 articles.

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2. Collapse of a molecular cloud core to stellar densities: the formation and evolution of pre-stellar discs

3. Evolution of rotating interstellar clouds. I - Numerical techniques

4. The Internal Energy for Molecular Hydrogen in Gravitationally Unstable Protoplanetary Disks

5. Ortho-para-hydrogen equilibration on Jupiter

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