Neutral and ionized hydrides in star-forming regions. Observations with Herschel/HIFI.

Abstract

The cosmic abundance of hydrides depends critically on high-energy UV, X-ray, and particle irradiation. Here we study hydrides in star-forming regions where irradiation by the young stellar object can be substantial, and density and temperature can be much enhanced over interstellar values. Lines of OH, CH, NH, and SH and their ions OH(+), CH(+), NH(+), SH… (More)
DOI: 10.1021/jp312813a

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