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Inter Stellar Shocked Region Chemistry Certain Reactions between Interstellar Molecules and O and N Atoms

Published online by Cambridge University Press:  04 August 2017

K. K. Ghosh ,
S. S. Saleem  and
K. N. Kutty
K. K. Ghosh
Affiliation:
Kavalur Observatory, Alangayam 635 701, India
S. S. Saleem
Affiliation:
Kavalur Observatory, Alangayam 635 701, India
K. N. Kutty
Affiliation:
Kavalur Observatory, Alangayam 635 701, India

Abstract

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The reactions between O and N atoms and certain interstellar molecules (H2S, NH3, H2CO, CH3 OH, C2 H5 OH) are studied using the dynamicalflowing after glow method. It is found that NH and OH radicals are formed which can be used as a diagnostic probe to differentiate between interstellar shocked and heated regions.

Type
Interstellar Medium
Information
Symposium - International Astronomical Union , Volume 120: Astrochemistry , 1987 , pp. 293 - 294
Copyright
Copyright © Reidel 1987 

References

1. Dalgarno, A., and Roberge, W.G. 1979, Ap. J. (Letters), 233, L25.CrossRefGoogle Scholar
2. Ghosh, S.N., Jain, S.K., and Gupta, S.K. 1962 Proc. Phys. Soc. (London) 79, 207.Google Scholar
3. Ghosh, K.K. 1984, Physica 124C, 395.Google Scholar
4. De Vos, J.C. 1954, Physica 20, 690.Google Scholar
5. Larrabee, R.D. 1959, J. Opt. Soc. Am. 49, 619.CrossRefGoogle Scholar