Skip navigation
Skip navigation

Ultrafaint dwarfs - Star formation and chemical evolution in the smallest galaxies

Webster, David; Sutherland, Ralph; Bland-Hawthorn, Joss

Description

In earlier work, we showed that a dark matter halo with a virial mass of 107 M ⊙ can retain a major part of its baryons in the face of the pre-ionization phase and supernova (SN) explosion from a 25 M ⊙ star. Here, we expand on the results of that wor

CollectionsANU Research Publications
Date published: 2014
Type: Journal article
URI: http://hdl.handle.net/1885/76040
Source: Astrophysical Journal, The
DOI: 10.1088/0004-637X/796/1/11

Download

File Description SizeFormat Image
01_Webster_Ultrafaint_dwarfs_-_Star_2014.pdf1.94 MBAdobe PDF    Request a copy


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