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SiO, (29)SiO, and (30)SiO emission from 67 oxygen-rich stars. A survey of 61 maser lines from 7 to 1 mm
Circumstellar environments of oxygen-rich stars are among the strongest SiO maser emitters. Physical processes such as collisions, infrared pumping and overlaps favors the inversion of level population and produce maser emission at different vibrational states. Despite numerous observational and the...
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| Publicado no: | Astrophys J Suppl Ser |
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| Main Authors: | , , |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
2021
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| Assuntos: | |
| Acesso em linha: | https://ncbi.nlm.nih.gov/pmc/articles/PMC7610587/ https://ncbi.nlm.nih.gov/pubmed/33854258 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.3847/1538-4365/abe469 |
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