Prospects of Searching for Type Ia Supernovae with 2.5-m Wide Field Survey Telescope

Type Ia Supernovae (SNe Ia) are the thermonuclear explosion of a carbon-oxygen white dwarf (WD) and are well-known as a distance indicator. However, it is still unclear how WDs increase their mass near the Chandrasekhar limit and how the thermonuclear runaway happens. The observational clues associa...

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Veröffentlicht in:	arXiv.org 2022-12
Hauptverfasser:	Hu, Maokai, Hu, Lei, Ji-an, Jiang, Lin, Xiao, Fan, Lulu, Wei, Junjie, Wu, Xuefeng
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Physics - High Energy Astrophysical Phenomena Physics - Solar and Stellar Astrophysics Supernovae Thermonuclear explosions White dwarf stars
Online-Zugang:	Volltext
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