Herschel/HIFI⋆ observations of the circumstellar ammonia lines in IRC+10216

CONTEXT: A discrepancy exists between the abundance of ammonia (NH(3)) derived previously for the circumstellar envelope (CSE) of IRC+10216 from far-IR submillimeter rotational lines and that inferred from radio inversion or mid-infrared (MIR) absorption transitions. AIMS: To address the discrepancy...

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發表在:Astron Astrophys
Main Authors: Schmidt, M. R., He, J. H., Szczerba, R., Bujarrabal, V., Alcolea, J., Cernicharo, J., Decin, L., Justtanont, K., Teyssier, D., Menten, K. M., Neufeld, D. A., Olofsson, H., Planesas, P., Marston, A. P., Sobolev, A. M., de Koter, A., Schöier, F. L.
格式: Artigo
語言:Inglês
出版: 2016
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Article
在線閱讀:https://ncbi.nlm.nih.gov/pmc/articles/PMC5217166/
https://ncbi.nlm.nih.gov/pubmed/28065983
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1051/0004-6361/201527290
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