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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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Bibliographic Details
Published in:Astrophys J Suppl Ser
Main Authors: Rizzo, J. R., Cernicharo, J., Garoía-Miró, C.
Format: Artigo
Language:Inglês
Published: 2021
Subjects:
Online Access: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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