Abundances of Light Metals in Field Stars with Metallicity Range - 1.2< [Fe/H]< + 0.3

Bibcode
1988IAUS..132..421A
Abia, C.; Rebolo, R.; Beckman, J. E.; Crivellari, L.; Vila, B.
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.421

Fecha de publicación:
0
1988
Número de autores
5
Número de autores del IAC
0
Número de citas
2
Número de citas referidas
2
Descripción
High resolution, high S:N spectra are used to determine the abundances of Fe, Ni, Ca, Al and Si in 25 field dwarfs with -1.2 < [Fe/H] < +0.3. The authors find overabundances for Al, Ca and Si in stars with -1.2 < [Fe/H] < -0.5 and solar [Ni/Fe] over the whole studied range.
Tipo
Sin árbitro

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