Bibcode
Bazan, J. J.; Molla, M.; Cerviño, & M.
Referencia bibliográfica
eprint arXiv:astro-ph/0302092
Fecha de publicación:
2
2003
Número de citas
0
Número de citas referidas
0
Descripción
Chemical abundance data for the Galaxy show a wide dispersion. We try to
check if this dispersion may also be found with chemical evolution
models as an effect of variations of an Initial Mass Function (IMF)
which follows a Poisson's distribution