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A Re-Evaluation of the Abundance of Lutetium in the Sun

โœ Scribed by D. J. Bord; C. R. Cowley; D. Mirijanian


Book ID
110217124
Publisher
Springer
Year
1998
Tongue
English
Weight
291 KB
Volume
178
Category
Article
ISSN
0038-0938

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๐Ÿ“œ SIMILAR VOLUMES


Abundance of Boron in the Sun
โœ LAMBERT, D. L.; MALLIA, E. A.; WARNER, B. ๐Ÿ“‚ Article ๐Ÿ“… 1966 ๐Ÿ› Nature Publishing Group ๐ŸŒ English โš– 191 KB
Abundance of Helium in the Sun
โœ LAMBERT, D. L. ๐Ÿ“‚ Article ๐Ÿ“… 1967 ๐Ÿ› Nature Publishing Group ๐ŸŒ English โš– 258 KB
The abundance of chlorine in the Sun
โœ D. L. Lambert; E. A. Mallia ๐Ÿ“‚ Article ๐Ÿ“… 1968 ๐Ÿ› Springer ๐ŸŒ English โš– 273 KB

The Cll line 2 8375.943 (4s aPs:,., 9 4p-."D%:,.) is identified in the solar spectrum. This is the tirst identification of a chlorine line in solar spectrum. The measured equivalent width (W;. --0.8 rnJk) corresponds to an abttndance IogN(Cl)-5.65 on the scale [ogN(H).. ]2.00.

The Abundance of Lead in the Sun
โœ John Ross, Lawrence H. Aller and Orren C. Mohler ๐Ÿ“‚ Article ๐Ÿ“… 1968 ๐Ÿ› National Academy of Sciences ๐ŸŒ English โš– 215 KB
Abundances of heavy elements in the sun
โœ Nicolas Grevesse ๐Ÿ“‚ Article ๐Ÿ“… 1969 ๐Ÿ› Springer ๐ŸŒ English โš– 777 KB

Solar abundances have been derived for Pb, Bi, Th and U. For the three lirst elements, the abundances are determined from the profiles of their lines obtained with the high resolution solar spectrometer installed at the Jungfraujoch Scientific Station (Switzerland) and fi'om new oscillator strengths