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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/323
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dc.contributor.authorTripathi, B. M-
dc.contributor.authorPande, M. C-
dc.date.accessioned2005-02-05T04:49:44Z-
dc.date.available2005-02-05T04:49:44Z-
dc.date.issued1981-12-
dc.identifier.citationBASI, Vol. 9, No. 4, pp. 287-290en
dc.identifier.urihttp://hdl.handle.net/2248/323-
dc.description.abstractAn attempt has been made to show that the profile of the Brackett-gamma line can distinguish between different facula models. It is suggested that low noise high resolution scans of Brackett lines can help improve the existing facula models.en
dc.format.extent258005 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjectBrackett lineen
dc.subjectfacula modelsen
dc.titleBrackett-gamma line and facula modelsen
dc.typeArticleen
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