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 |