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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1915
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dc.contributor.authorStalin, C. S-
dc.contributor.authorSinha, K-
dc.contributor.authorSanwal, B. B-
dc.date.accessioned2007-10-19T12:13:42Z-
dc.date.available2007-10-19T12:13:42Z-
dc.date.issued1997-
dc.identifier.citationBASI, Vol. 25, No. 1, pp. 117 - 132en
dc.identifier.urihttp://hdl.handle.net/2248/1915-
dc.description.abstractUtilizing Lieze solar atlas and solar photospheric models, we derived log gf values for the spectral lines in the wavelength range λλ 6209 - 6273 Å. These values, intended for use in a future study of high resolution reticon spectrum of the star gamma Draconis, are presented along with some recent results available in the literatureen
dc.format.extent1224211 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1997BASI...25..117Sen
dc.subjectOscillator strengthsen
dc.subjectPhotospheric modelsen
dc.subjectSolar spectrumen
dc.titleSolar log gf values for the spectral lines in the range λ λ 6209-6273 Åen
dc.typeArticleen
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