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A method of evaluating the abundances of heavy elements in metal-poor stars

โœ Scribed by Bo Zhang; Ji Li; Cai-xia Zhang; Yan-chun Liang; Qiu-he Peng


Book ID
108427676
Publisher
Elsevier Science
Year
2000
Tongue
English
Weight
561 KB
Volume
24
Category
Article
ISSN
0275-1062

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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