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Segregation of the heavy elements in the solar system

โœ Scribed by I. P. Williams; M. J. Handbury


Publisher
Springer Netherlands
Year
1974
Tongue
English
Weight
427 KB
Volume
30
Category
Article
ISSN
0004-640X

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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