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Spectroscopic constraints on CH(3)OH formation: CO mixed with CH(3)OH ices towards young stellar objects
The prominent infrared absorption band of solid CO – commonly observed towards young stellar objects (YSOs) – consists of three empirically determined components. The broad ‘red component’ (2136 cm(−1), 4.681 μm) is generally attributed to solid CO mixed in a hydrogen-bonded environment. Usually, CO...
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| Pubblicato in: | Mon Not R Astron Soc |
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| Autori principali: | , , , , , |
| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
2015
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| Soggetti: | |
| Accesso online: | https://ncbi.nlm.nih.gov/pmc/articles/PMC6893920/ https://ncbi.nlm.nih.gov/pubmed/31806918 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1093/mnras/stv1987 |
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