Smith, M.D., Pavlovski, G., Maclow, M.-M., Rosen, A., Khanzadyan, T., Gredel, R., Stanke, T. (2004) Molecule destruction and formation in molecular clouds. Astrophysics and Space Science, 289 (3-4). pp. 333-336. ISSN 0004-640X. (doi:10.1023/B:ASTR.0000014962.69571.e5) (The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided) (KAR id:50123)
| The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided. | |
| Official URL: http://dx.doi.org/10.1023/B:ASTR.0000014962.69571.... |
Abstract
We show that supersonic turbulence accelerates the transition of an atomic cloud into a molecular cloud, quantified here through a demo model and 3D numerical simulations which explicitly include atomic-molecular chemistry. Specific sites where amplified formation may be detectable are suggested.
| Item Type: | Article |
|---|---|
| DOI/Identification number: | 10.1023/B:ASTR.0000014962.69571.e5 |
| Subjects: | Q Science > QB Astronomy > QB460 Astrophysics |
| Divisions: | Divisions > Division of Natural Sciences > Physics and Astronomy |
| Depositing User: | Giles Tarver |
| Date Deposited: | 11 Aug 2015 09:43 UTC |
| Last Modified: | 05 Nov 2024 10:35 UTC |
| Resource URI: | https://kar.kent.ac.uk/id/eprint/50123 (The current URI for this page, for reference purposes) |
University of Kent Author Information
Smith, M.D..
| Creator's ORCID: |
 https://orcid.org/0000-0002-4289-5952
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