The Pisa pre-‐MS tracks and isochrones
Asteroseismic age estimates of RGB stars in open clusters - A statistical investigation of different estimation methods
Pre-Main Sequence evolutionary models (low and intermediate mass) Scilla Degl'Innocenti Emanuele Tognelli Pier Giorgio Prada Moroni (Physics Department, - ppt download
arXiv:1510.02620v1 [astro-ph.SR] 9 Oct 2015
Theoretical uncertainties on classical Cepheid pulsational quantities
Appunti Fisica
Pier Giorgio PRADA MORONI | Associate professor | Ph. D. in Physics | Università di Pisa, Pisa | UNIPI | Department of Physics "E.Fermi"
Frontiers | Theoretical Predictions of Surface Light Element Abundances in Protostellar and Pre-Main Sequence Phase
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Galactic structure and white dwarf populations
Pier Giorgio PRADA MORONI | Associate professor | Ph. D. in Physics | Università di Pisa, Pisa | UNIPI | Department of Physics "E.Fermi"
Effect of planet ingestion on low-mass stars evolution: The case of 2MASS J08095427-4721419 star in the Gamma Velorum cluster
Scoperta una nuova classe di stelle all'Università di Pisa
Pisa Stellar Models
PDF) Recovering the star formation rate in the solar neighborhood | S. Degl'Innocenti - Academia.edu
Pier Giorgio PRADA MORONI | Associate professor | Ph. D. in Physics | Università di Pisa, Pisa | UNIPI | Department of Physics "E.Fermi"
Consortium Members
Pier Giorgio PRADA MORONI | Associate professor | Ph. D. in Physics | Università di Pisa, Pisa | UNIPI | Department of Physics "E.Fermi"
arXiv:astro-ph/0702405v1 15 Feb 2007
Mixing-Length Estimates From Binary Systems. A Theoretical Investigation on the Estimation Errors
