The solar abundance of gold

descriptionPublicationkeyboard_double_arrow_right Article 01 Mar 1972 English Publisher:Springer Science and Business Media LLCJournal:Solar Physics, volume 23, pages 13-17 (issn: 0038-0938, eissn: 1573-093X,

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Authors: John E. Ross; Lawrence H. Aller;

doi: 10.1007/bf00153887

The solar abundance of gold

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Abstract

From 13 scans obtained with a double-band pass spectrograph at the Snow telescope at Mount Wilson, interpreted by the method of spectral synthesis, the abundance of gold turns out to be log [N(Au)/N(H)] + 12 = 0.70, assuming loggf = − 0.57.

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University of California, Los Angeles
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