Skip navigation
Skip navigation

Modelling the Pan-Spectral Energy Distribution of Starburst Galaxies: The role of ISM pressure and the Molecular Cloud Dissipation Timescale

CollectionsANU Research Publications
Date published: 2004
Type: Conference paper
URI: http://hdl.handle.net/1885/80872
Source: Asronomische Nachriten/Astronomical Notes vol. 325 Supp. Issue 1

Download

There are no files associated with this item.


Items in Open Research are protected by copyright, with all rights reserved, unless otherwise indicated.

Updated:  20 July 2017/ Responsible Officer:  University Librarian/ Page Contact:  Library Systems & Web Coordinator