investigation of Stars In the Milky way with Bayesian statistics and Asteroseismology
V. Grisoni, E. Spitoni, F. Matteucci
Abundance gradients along the Galactic disc from chemical evolution models
See arXiv version
12 pages, 7 figures. Accepted for publication in MNRAS
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Spitoni, Emanuele;, Vincenzo, Fiorenzo;, Matteucci, Francesca;, Romano, Donatella
Origin of the Galactic Halo: accretion vs. in situ formation
Rediscovering our Galaxy, Proceedings of the International Astronomical Union, IAU Symposium
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C. De Masi, F. Vincenzo, F. Matteucci, G. Rosani, La Barbera, A. Pasquali, E. Spitoni
Is the IMF in ellipticals bottom-heavy? Clues from their chemical abundances
See arXiv version
24 pages, 25 figures, accepted for publication on MNRAS
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