Uncertainties in stellar ages provided by grid techniques
arXiv:1510.02620v1 [astro-ph.SR] 9 Oct 2015
Scoperta una nuova classe di stelle all'Università di Pisa
Pier Giorgio PRADA MORONI | Associate professor | Ph. D. in Physics | Università di Pisa, Pisa | UNIPI | Department of Physics "E.Fermi"
White Dwarfs and Fundamental Physics: P. G. Prada Moroni | PDF | Stars | Gases
Theoretical uncertainties on white dwarf luminosity functions
7Li surface abundance in pre-main sequence stars
PDF) Recovering the star formation rate in the solar neighborhood | S. Degl'Innocenti - Academia.edu
Effect of planet ingestion on low-mass stars evolution: The case of 2MASS J08095427-4721419 star in the Gamma Velorum cluster
Pier Giorgio Prada Moroni
The Pisa pre-‐MS tracks and isochrones
Pier Giorgio PRADA MORONI | Associate professor | Ph. D. in Physics | Università di Pisa, Pisa | UNIPI | Department of Physics "E.Fermi"
2018 Spring Symposia - April 23-26 - Booklet
Pre-Main Sequence evolutionary models (low and intermediate mass) Scilla Degl'Innocenti Emanuele Tognelli Pier Giorgio Prada Moroni (Physics Department, - ppt download
arXiv:astro-ph/0405101v1 6 May 2004
Pier Giorgio PRADA MORONI | Associate professor | Ph. D. in Physics | Università di Pisa, Pisa | UNIPI | Department of Physics "E.Fermi"
arXiv:1605.07920v1 [astro-ph.SR] 25 May 2016
The Pisa pre-‐MS tracks and isochrones
Frontiers | Theoretical Predictions of Surface Light Element Abundances in Protostellar and Pre-Main Sequence Phase
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Pier Giorgio PRADA MORONI | Associate professor | Ph. D. in Physics | Università di Pisa, Pisa | UNIPI | Department of Physics "E.Fermi"
Galactic structure and white dwarf populations
