The solar platinum content

Details The solar platinum content The solar platinum content

Nov 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...186..333y&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 186, no. 1-2, Nov. 1987, p. 333, 334.

Astronomy and Astrophysics

Astrophysics

4

Abundance, Platinum, Solar Spectra, Stellar Composition, Laser Induced Fluorescence, Line Spectra, Oscillator Strengths, Photosphere, Radiative Lifetime, Ultraviolet Spectra

Scientific paper

Using the spectral synthesis method with the Holweger-Müller solar model atmosphere, the solar abundance of platinum is derived from an LTE analysis of the photospheric spectrum. The recent value of the oscillator strength, deduced from lifetime measurements is used. The authors obtain APt = 1.74 in the usual scale where log AH = 12.00.

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