Smith, Michael D., Rosen, Alexander (2005) Hydrodynamic simulations of molecular outflows driven by slow precessing protostellar jets. Monthly Notices of the Royal Astronomical Society, 357 . pp. 579-589. ISSN 0035-8711. (doi:10.1111/j.1365-2966.2005.08678.x) (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:1146)
| 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: https://doi.org/10.1111/j.1365-2966.2005.08678.x |
Abstract
As part of an extensive programme to understand how stars can form, Smith performed large-scale computer simulations. While there have been many studies of astrophysical phenomena on computers, few have processed the images through numerical telescopes to reveal the observable structure and so provide an interface between observation and theory. this work provided an extensive study of one of the most observationally indicated properties. The paper set the scene for international collaborations in order to compare to data to observations. (Impact Factor: 5.352)
| Item Type: | Article |
|---|---|
| DOI/Identification number: | 10.1111/j.1365-2966.2005.08678.x |
| Subjects: |
Q Science > Q Science (General) Q Science > QB Astronomy Q Science > QC Physics |
| Divisions: | Divisions > Division of Natural Sciences > Physics and Astronomy |
| Depositing User: | Sara Witchell |
| Date Deposited: | 19 Dec 2007 18:45 UTC |
| Last Modified: | 05 Nov 2024 09:31 UTC |
| Resource URI: | https://kar.kent.ac.uk/id/eprint/1146 (The current URI for this page, for reference purposes) |
University of Kent Author Information
Smith, Michael D..
| Creator's ORCID: |
 https://orcid.org/0000-0002-4289-5952
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