Subaru High-Resolution Spectroscopy of Star G in the Tycho Supernova Remnant
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Kerzendorf, Wolfgang
Schmidt, Brian
Asplund, Martin
Nomoto, Ken'ichi
Podsiadlowski, Ph.
Frebel, Anna
Fesen, Robert A
Yong, David
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IOP Publishing
Abstract
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
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Astrophysical Journal, The
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