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Ionised molecules in BCA photospheric model

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dc.contributor.author Pande, M. C.
dc.contributor.author Gaur, V. P.
dc.date.accessioned 2011-12-15T05:10:04Z
dc.date.available 2011-12-15T05:10:04Z
dc.date.issued 1972
dc.identifier.uri http://hdl.handle.net/123456789/883
dc.description.abstract The dissociation equilibrium of ionized diatomic molecular species CO⁺, N O⁺, OH⁺, O₂⁺, N₂⁺, H₂⁺ in BCA photospheric model is considered. The abundances of these species are in the order H₂⁺, CO⁺, OH⁺, NO⁺, O₂⁺ and N₂⁺. the equivalent width of R (K=30) line of the (0-3) band belonging to the transition A ² ∏I - X²∑⁺ of CO⁺ is either 0.042 or 0.084 mA (cf.text) which shows that no detectible lines of CO⁺ occur in the photospheric spectrum. en_US
dc.language.iso en_US en_US
dc.relation.ispartofseries bac24-207
dc.subject BCA Photospheric en_US
dc.title Ionised molecules in BCA photospheric model en_US
dc.type Article en_US


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