Bibcode
Arribas, S.; Martinez-Roger, C.
Referencia bibliográfica
The Impact of Very High S/N Spectroscopy on Stellar Physics: Proceedings of the 132nd Symposium of the International Astronomical Union held in Paris, France, June 29-July 3, 1987. Edited by G. Cayrel de Strobel and Monique Spite. International Astronomical Union. Symposium no. 132, Kluwer Academic Publishers, Dordrecht., p.445
Fecha de publicación:
0
1988
Número de citas
2
Número de citas referidas
2
Descripción
The authors present a spectroscopic analysis for the gravity
determination of τ Ceti on the basis of a new and high quality set
of data. The iron lines are studied by using the Oxford oscillator
strengths. The results are compared with those obtained with "solar"
oscillator strengths. Non-LTE effects seem to be important in this star.
The Fe I at λ526.955 nm line is used to apply the Blackwell and
Willis (1977) method to determine the surface gravity. The derived log g
is 4.70±0.1.