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Producing type Ia supernovae from hybrid CONe white dwarfs with main-sequence binary companions at low metallicity of Z = 0.0001

Fuente: arXiv

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Dettagli Bibliografici
Autori principali:	Guo, Boyang, Meng, Xiangcun, Tian, Zhijia, Luo, Jingxiao, Liu, Zhengwei
Natura:	Preprint
Pubblicazione:	2025
Soggetti:	Solar and Stellar Astrophysics High Energy Astrophysical Phenomena
Accesso online:	Acceder al recurso
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