1. Photochemical origin of SiC$_2$ in the circumstellar envelope of carbon-rich AGB stars revealed by ALMA
- Author
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Feng, Yanan, Li, Xiaohu, Millar, Tom J., Szczerba, Ryszard, Wang, Ke, Quan, Donghui, Qin, Shengli, Fang, Xuan, Tuo, Juan, Miao, Zhenzhen, Ma, Rong, Xu, Fengwei, Sun, Jingfei, Jiang, Biwei, Chang, Qiang, Yang, Jianchao, Hou, Gao-Lei, Li, Fangfang, and Zhang, Yong
- Subjects
Astrophysics - Solar and Stellar Astrophysics ,Astrophysics - Astrophysics of Galaxies - Abstract
Whether SiC$_2$ is a parent species, that is formed in the photosphere or as a by-product of high-temperature dust formation, or a daughter species, formed in a chemistry driven by the photodestruction of parent species in the outer envelope, has been debated for a long time. Here, we analyze the ALMA observations of four SiC$_2$ transitions in the CSEs of three C-rich AGB stars (AI Vol, II Lup, and RAFGL 4211), and found that SiC$_2$ exhibits an annular, shell-like distribution in these targets, suggesting that SiC$_2$ can be a daughter species in the CSEs of carbon-rich AGB stars. The results can provide important references for future chemical models., Comment: Accepted in Frontiers in Astronomy and Space Sciences
- Published
- 2023