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Observations of Molecular CN toward S-type Asymptotic Giant Branch Stars

S-type asymptotic giant branch (AGB) stars are defined by their carbon-to-oxygen (C/O) ratio approaching unity. However, observations of circumstellar molecules in these stars are limited and challenging. In this study, we used the James Clerk Maxwell Telescope to search for cyanide (CN) in 12 selec...

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Principais autores: Yanan Feng, Xiaohu Li, Xiaofeng Yang, Tom J. Millar, Ryszard Szczerba, Sheng-Li Qin, Xuejian Jiang, Donghui Quan, Juan Tuo, Zhenzhen Miao, Sheng-Yuan Liu, Xiang Liu
פורמט: Artigo
שפה:Inglês
יצא לאור: IOP Publishing 2024-01-01
סדרה:The Astronomical Journal
נושאים:
Asymptotic giant branch
Circumstellar envelopes
Astrochemistry
גישה מקוונת:https://doi.org/10.3847/1538-3881/ad8ba6
תגים: הוספת תג
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