Modelling H2 formation in the turbulent interstellar medium: solenoidal versus compressive turbulent forcing
Article first published online: 23 FEB 2012
© 2012 The Authors Monthly Notices of the Royal Astronomical Society © 2012 RAS
Monthly Notices of the Royal Astronomical Society
Volume 421, Issue 3, pages 2531–2542, April 2012
How to Cite
Micic, M., Glover, S. C. O., Federrath, C. and Klessen, R. S. (2012), Modelling H2 formation in the turbulent interstellar medium: solenoidal versus compressive turbulent forcing. Monthly Notices of the Royal Astronomical Society, 421: 2531–2542. doi: 10.1111/j.1365-2966.2012.20477.x
- Issue published online: 4 APR 2012
- Article first published online: 23 FEB 2012
- Accepted 2012 January 3. Received 2011 December 30; in original form 2011 March 10
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