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

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Date

Authors

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

Journal Title

Journal ISSN

Volume Title

Publisher

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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Citation

Source

Astrophysical Journal, The

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Entity type

Access Statement

Open Access

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Restricted until

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