dc.contributor.author | Tripathi, B. M | |
dc.contributor.author | Gaur, V. P | |
dc.contributor.author | Pande, M. C | |
dc.date.accessioned | 2005-02-04T16:41:14Z | |
dc.date.available | 2005-02-04T16:41:14Z | |
dc.date.issued | 1981-09 | |
dc.identifier.citation | BASI, Vo. 9, No. 3, pp. 227-231 | en |
dc.identifier.uri | http://hdl.handle.net/2248/316 | |
dc.description.abstract | Equivalent 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.extent | 385312 bytes | |
dc.format.mimetype | application/pdf | |
dc.language.iso | en | |
dc.publisher | Astronomical Society of India | en |
dc.subject | ionized molecules | en |
dc.subject | equivalent widths | en |
dc.subject | facula models | en |
dc.title | Ionized molecules in facula models | en |
dc.type | Article | en |