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astro-ph2004
Models of Stellar structure for asteroseismology
F. D'Antona, J. Montalban, I. Mazzitelli
Among the problems still open in the study of stellar structure, we discuss in particular some issues related to the study of convection. We have recently built up complete stellar…
astro-ph2004★ 7 cited
Solar model with CNO revised abundances
J. Montalban, A. Miglio, A. Noels +3
Recent three-dimensional, NLTE analyses of the solar spectrum have shown a significant reduction in the C, N, O and Ne abundances leading to a Z/X ratio of the order of 0.0177. We…