Phillips, T. G. and van Dishoeck, Ewine F. and Keene, Jocelyn B. (1992) Interstellar H₃O⁺. In: Astrochemistry of Cosmic Phenomena. International Astronomical Union Symposium (IAUS). No.150. Springer Netherlands , Dordrecht, pp. 191-192. ISBN 9780792318255. https://resolver.caltech.edu/CaltechAUTHORS:20201023-102057324
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Abstract
The H₃O⁺ ion is a key species in the oxygen chemistry leading to H₂O, OH and O₂. Chemical models predict O₂ and H₂O to be the dominant oxygen-bearing molecules in interstellar clouds. However, neither of them can easily be observed in the bulk of the interstellar medium because of blockage from the Earth’s atmosphere. Determination of the abundance and distribution of the precursor H₃O⁺ ion might thus provide an important indirect measure of their abundances.
| Item Type: | Book Section | |||||||||
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| Additional Information: | © Springer Science+Business Media Dordrecht 1992. | |||||||||
| Series Name: | International Astronomical Union Symposium (IAUS) | |||||||||
| Issue or Number: | 150 | |||||||||
| DOI: | 10.1007/978-94-011-2761-5_44 | |||||||||
| Record Number: | CaltechAUTHORS:20201023-102057324 | |||||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20201023-102057324 | |||||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | |||||||||
| ID Code: | 106250 | |||||||||
| Collection: | CaltechAUTHORS | |||||||||
| Deposited By: | George Porter | |||||||||
| Deposited On: | 23 Oct 2020 21:10 | |||||||||
| Last Modified: | 16 Nov 2021 18:52 |
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