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Revised spectroscopic parameters of SH(+) from ALMA() and IRAM 30m() observations()
Hydrides represent the first steps of interstellar chemistry. Sulfanylium (SH(+)), in particular, is a key tracer of energetic processes. We used ALMA and the IRAM 30 m telescope to search for the lowest frequency rotational lines of SH(+) toward the Orion Bar, the prototypical photo-dissociation re...
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| Publié dans: | Astron Astrophys |
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| Auteurs principaux: | , , , , , , , , |
| Format: | Artigo |
| Langue: | Inglês |
| Publié: |
2014
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| Sujets: | |
| Accès en ligne: | https://ncbi.nlm.nih.gov/pmc/articles/PMC4623156/ https://ncbi.nlm.nih.gov/pubmed/26525172 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1051/0004-6361/201424756 |
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