Subaru High-Resolution Spectroscopy of Star G in the Tycho Supernova Remnant
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
|Collections||ANU Research Publications|
|Source:||Astrophysical Journal, The|
|01_Kerzendorf_Subaru_High-Resolution_2009.pdf||729.27 kB||Adobe PDF|
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