dc.contributor.author |
Stalin, C. S |
|
dc.contributor.author |
Sinha, K |
|
dc.contributor.author |
Sanwal, B. B |
|
dc.date.accessioned |
2007-10-19T12:13:42Z |
|
dc.date.available |
2007-10-19T12:13:42Z |
|
dc.date.issued |
1997 |
|
dc.identifier.citation |
BASI, Vol. 25, No. 1, pp. 117 - 132 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/1915 |
|
dc.description.abstract |
Utilizing 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 literature |
en |
dc.format.extent |
1224211 bytes |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en |
en |
dc.publisher |
Astronomical Society of India |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/1997BASI...25..117S |
en |
dc.subject |
Oscillator strengths |
en |
dc.subject |
Photospheric models |
en |
dc.subject |
Solar spectrum |
en |
dc.title |
Solar log gf values for the spectral lines in the range λ λ 6209-6273 Å |
en |
dc.type |
Article |
en |