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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

Description

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
URI: http://hdl.handle.net/1885/31537
Source: Astrophysical Journal, The
DOI: 10.1088/0004-637X/701/2/1665

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