Galactic Evolution of Beryllium and Oxygen

Bibcode
2000IAUS..198..397I
Israelian, G.; López, R. J. G.; Rebolo, R.
Referencia bibliográfica

The Light Elements and their Evolution, Proceedings of IAU Symposium 198, held 22-26 Nov 1999, Natal, Brazil. Edited by L. da silva, R. de Medeiros, &M Spite, 2000., p.397

Fecha de publicación:
0
2000
Número de autores
3
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
We discuss the early evolution of beryllium and oxygen in our Galaxy by comparing abundances of these elements for halo and disk metal-poor stars. Both, O and Be rise as we go progressively to more metal-rich stars, showing a slope 0.41 +-0.09 ([Be/O] vs [Fe/H]) for stars with [Fe/H] < -1. This relationship provides an observational constraint to the actually proposed Galactic Cosmic Ray theories.
Tipo
Sin árbitro

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