An interstellar line coincident with the P(2,l)transition of hydronium (H3O+)
- 1 August 1986
- journal article
- letter
- Published by Springer Nature in Nature
- Vol. 322 (6079) , 524-526
- https://doi.org/10.1038/322524a0
Abstract
No abstract availableKeywords
This publication has 10 references indexed in Scilit:
- Rate coefficients of the reactions of ions with polar molecules at interstellar temperaturesThe Astrophysical Journal, 1985
- Laboratory measurement of the P(2,1) submillimeter transition frequency of H3O+The Journal of Chemical Physics, 1985
- Synthesis of complex molecules in dense interstellar clouds via gas-phase chemistry - A pseudo time-dependent calculationThe Astrophysical Journal Supplement Series, 1984
- Interaction of the outflow and quiescent gas in Orion - HCO(+) aperture synthesis mapsThe Astrophysical Journal, 1984
- Spectroscopic properties of the hydroxonium ion calculated from scep cepa wavefunctionsChemical Physics Letters, 1983
- Kinematics of Orion-KL - Aperture synthesis maps of 86 GHz SO emissionThe Astrophysical Journal, 1982
- Metastable isomers - A new class of interstellar moleculesThe Astrophysical Journal, 1979
- Indirect observation of unobservable interstellar moleculesThe Astrophysical Journal, 1977
- CO and CS in the Orion NebulaThe Astrophysical Journal, 1974
- The Formation and Depletion of Molecules in Dense Interstellar CloudsThe Astrophysical Journal, 1973