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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/316
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dc.contributor.authorTripathi, B. M-
dc.contributor.authorGaur, V. P-
dc.contributor.authorPande, M. C-
dc.date.accessioned2005-02-04T16:41:14Z-
dc.date.available2005-02-04T16:41:14Z-
dc.date.issued1981-09-
dc.identifier.citationBASI, Vo. 9, No. 3, pp. 227-231en
dc.identifier.urihttp://hdl.handle.net/2248/316-
dc.description.abstractEquivalent widths for the lines of ionized molecules AlH+, CH+, CN+ CO+, 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 AlH+, CN+, CO+, N2+ should be absent.en
dc.format.extent385312 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjectionized moleculesen
dc.subjectequivalent widthsen
dc.subjectfacula modelsen
dc.titleIonized molecules in facula modelsen
dc.typeArticleen
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