Skip navigation
Skip navigation

Subaru High-Resolution Spectroscopy of Star G in the Tycho Supernova Remnant

Kerzendorf, Wolfgang; Schmidt, Brian; Asplund, Martin; Nomoto, Ken'ichi; Podsiadlowski, Ph.; Frebel, Anna; Fesen, Robert A; Yong, David


It is widely believed that Type Ia supernovae (SNe Ia) originate in binary systems where a white dwarf accretes material from a companion star until its mass approaches the Chandrasekhar mass and carbon is ignited in the white dwarf's core. This scenario

CollectionsANU Research Publications
Date published: 2009
Type: Journal article
Source: Astrophysical Journal, The
DOI: 10.1088/0004-637X/701/2/1665


File Description SizeFormat Image
01_Kerzendorf_Subaru_High-Resolution_2009.pdf729.27 kBAdobe PDF

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

Updated:  22 January 2019/ Responsible Officer:  University Librarian/ Page Contact:  Library Systems & Web Coordinator