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Detailed Analyses of Four Solar Analogs Analysed On High S/N CFH and ESO Spectra

Published online by Cambridge University Press:  19 July 2016

C. Bentolila  and
G. Cayrel de Strobel
C. Bentolila
Affiliation:
Observatoire de Paris, Section de Meudon, F-92195, Meudon Cedex, France
G. Cayrel de Strobel
Affiliation:
Observatoire de Paris, Section de Meudon, F-92195, Meudon Cedex, France

Abstract

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Four solar type G stars claimed to be photometrically very similar to the Sun have been analyzed in detail on high resolution, high S/N spectra. Their atmospheric parameters : effective temperature, spectroscopic gravity, microturbulence and iron abundance, [Fe/H], have been determined.

Type
VI. Chemical Composition of Stars
Information
Symposium - International Astronomical Union , Volume 132: The Impact of Veryhigh S/N Spectroscopy on Stellar Physics , 1988 , pp. 429 - 432
Copyright
Copyright © Kluwer 1988 

References

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