dc.contributor.author | Tripathi, B. M. | |
dc.contributor.author | Gaur, V. P. | |
dc.contributor.author | Pande, M. C. | |
dc.date.accessioned | 2010-08-20T09:44:42Z | |
dc.date.available | 2010-08-20T09:44:42Z | |
dc.date.issued | 1981 | |
dc.identifier.citation | This article downloaded from ADS | en_US |
dc.identifier.uri | http://hdl.handle.net/123456789/749 | |
dc.description.abstract | Equivalent widths for the lines of ionized molecules A1H⁺, CH⁺, CN⁺, CO⁺, MgH⁺, N2⁺, NH⁺, OH⁺ and SiH⁺ have been calculated in five facular and two photospheric models. The calculations suggest that CH⁺ should show up in facular spectrum. MgH⁺, OH⁺ and SiH⁺ may also be present while A1H⁺, CN⁺, CO⁺, N2⁺ and NH⁺ should be absent. | en_US |
dc.language.iso | en_US | en_US |
dc.relation.ispartofseries | basi9-227 | |
dc.subject | Ionized molecules, Equivalent widths, Facula models | en_US |
dc.title | Ionized Molecules in facula models | en_US |
dc.type | Article | en_US |