Physics
Scientist
Oxford University, Oxford, England
Interpretation of the solar spectrum 300 NM to 900 nm. I - Fe I lines of excitation potential 0.00 eV-0.12 eV microturbulence, damping, abundance, tests of oscillator strengths
Precision measurement of relative oscillator strengths. III - Fe I transitions from levels a5D2 /0.09 eV/, a5D1 /0.11 eV/, and a5D0 /0.12 eV/
Some values of delta S for RR Lyrae stars
Stellar gravities from metallic line profiles, with application to Arcturus - The effective temperature of Arcturus
The continuum flux distribution for Arcturus
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