Solar log gf values for the spectral lines in the range  λλ 6209-6273 Å

dc.contributor.author	Stalin, C. S.
dc.contributor.author	Sinha, K.
dc.contributor.author	Sanwal, B. B.
dc.date.accessioned	2009-12-17T04:35:34Z
dc.date.available	2009-12-17T04:35:34Z
dc.date.issued	1997
dc.identifier.citation	This article downloded from ADS Free Online Journal	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/377
dc.description.abstract	Utilizing Liege 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 a high resolution reticon spectrum of the star ϒ Draconis, are presented along with some recent results available in the literature.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	basi25-117
dc.subject	Log gf, Oscillator strengths, Photospheric models, Solar systems	en_US
dc.title	Solar log gf values for the spectral lines in the range λλ 6209-6273 Å	en_US
dc.type	Article	en_US