Smith, Michael D., Rosen, Alexander (2005) Synthetic Spitzer Infrared Array Camera Band Maps from Simulations of Protostellar jets. Monthly Notices of the Royal Astronomical Society, 357 . pp. 1370-1376. ISSN 0035-8711. (doi:10.1111/j.1365-2966.2005.08785.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:1147)
| 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/10.1111/j.1365-2966.2005.08785.x |
Abstract
This work was led by Smith in order to make the best use of a new satellite, the Spitzer space telescope, with which he is a co-investigator on several observational campaigns. In this paper, we analysed bow shocks and computer simulations of protostellar jets to extract predictions for how Spitzer would observe to outflowing material. It provides essential predictions, since confirmed in all observations of outflows. (Impact Factor: 5.352)
| Item Type: | Article |
|---|---|
| DOI/Identification number: | 10.1111/j.1365-2966.2005.08785.x |
| Subjects: |
Q Science 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/1147 (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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