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Circumstellar chemistry of Si-C bearing molecules in the C-rich AGB star IRC+10216
Silicon carbide together with amorphous carbon are the main components of dust grains in the atmospheres of C-rich AGB stars. Small gaseous Si-C bearing molecules (such as SiC, SiCSi, and SiC(2)) are efficiently formed close to the stellar photosphere. They likely condense onto dust seeds owing to t...
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| Pubblicato in: | Proc Int Astron Union |
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| Autori principali: | , , , , , , , , , , , , , |
| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
2019
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| Soggetti: | |
| Accesso online: | https://ncbi.nlm.nih.gov/pmc/articles/PMC6944505/ https://ncbi.nlm.nih.gov/pubmed/31908652 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1017/S1743921318005410 |
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