Hydrodynamic simulations of molecular outflows driven by slow precessing protostellar jets

Smith, Michael D. and 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. (The full text of this publication is not available from this repository)

The full text of this publication is not available from this repository. (Contact us about this Publication)

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
Subjects: Q Science > Q Science (General)
Q Science > QB Astronomy
Q Science > QC Physics
Divisions: Faculties > Science Technology and Medical Studies > School of Physical Sciences
Depositing User: Sara Witchell
Date Deposited: 19 Dec 2007 18:45
Last Modified: 09 Jun 2014 09:26
Resource URI: http://kar.kent.ac.uk/id/eprint/1146 (The current URI for this page, for reference purposes)
  • Depositors only (login required):