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Hunting for the progenitor of SN 1006: High-resolution spectroscopic search with the flames instrument

Kerzendorf, Wolfgang; Schmidt, Brian; Laird, J.B.; Podsiadlowski, Ph.; Bessell, Michael


Type Ia supernovae play a significant role in the evolution of the universe and have a wide range of applications. It is widely believed that these events are the thermonuclear explosions of carbon-oxygen white dwarfs close to the Chandrasekhar mass (1.38 M⊙). However, CO white dwarfs are born with masses much below the Chandrasekhar limit and thus require mass accretion to become Type Ia supernovae. There are two main scenarios for accretion: first, the merger of two white dwarfs and, second,...[Show more]

CollectionsANU Research Publications
Date published: 2012
Type: Journal article
Source: Astrophysical Journal, The
DOI: 10.1088/0004-637X/759/1/7


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