Please use this identifier to cite or link to this item: http://nopr.niscpr.res.in/handle/123456789/36779
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dc.contributor.authorGhosh, S N-
dc.contributor.authorGhosh, K K-
dc.date.accessioned2016-11-04T09:13:40Z-
dc.date.available2016-11-04T09:13:40Z-
dc.date.issued1982-02-
dc.identifier.issn0975-105X (Online); 0367-8393 (Print)-
dc.identifier.urihttp://nopr.niscair.res.in/handle/123456789/36779-
dc.description40-41en_US
dc.description.abstractUnlike neutral-neutral reactions which are mainly endothermic, most of the ion-neutral reactions in the interstellar space are exothermic. The energy released by the reaction of the latter type is less than the dissociation energy of the molecule. Such reactions may play dominant role in the interstellar medium. The information regarding the rate coefficients of polyatomic ionneutral reactions is meagre. A semi-classical approach is adopted here for calculating rate coefficient and its temperature dependence. The coefficients of certain important ion-neutral reactions in the interstellar medium are calculated and presented.en_US
dc.language.isoen_USen_US
dc.publisherNISCAIR-CSIR, Indiaen_US
dc.rights CC Attribution-Noncommercial-No Derivative Works 2.5 Indiaen_US
dc.sourceIJRSP Vol.11(1) [February 1982]en_US
dc.titleRate Coefficients of Some Important Interstellar lon-Neutral Reactionsen_US
dc.typeArticleen_US
Appears in Collections:IJRSP Vol.11(1) [February 1982]

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