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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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Autores principales: 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
Formato: Artigo
Lenguaje:Inglês
Publicado: IOP Publishing 2024-01-01
Colección:The Astronomical Journal
Materias:
Asymptotic giant branch
Circumstellar envelopes
Astrochemistry
Acceso en línea:https://doi.org/10.3847/1538-3881/ad8ba6
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