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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1459
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dc.contributor.authorGaur, V. P-
dc.contributor.authorJoshi, G. C-
dc.contributor.authorPande, M. C-
dc.date.accessioned2007-03-21T06:52:58Z-
dc.date.available2007-03-21T06:52:58Z-
dc.date.issued1992-
dc.identifier.citationBASI, Vol. 20, pp. 61-63en
dc.identifier.urihttp://hdl.handle.net/2248/1459-
dc.description.abstractThe equivalent widths of the P and R branch lines of the fundamental vibration-rotation band arising from the ground state of HeH(+) have been calculated in a chosen photospheric model. The resulting equivalent widths suggest that the solar spectrum in the infrared region should be searched for, resolving the question regarding the presence or absence of HeH(+) in the sunen
dc.format.extent248015 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectSolar spectraen
dc.titleCan HeH(+) molecule be present in solar photosphereen
dc.typeArticleen
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