arXiv:astro-ph/0702405v1 15 Feb 2007
Theoretical uncertainties on white dwarf luminosity functions
Asteroseismic age estimates of RGB stars in open clusters - A statistical investigation of different estimation methods
Scoperta una nuova classe di stelle all'Università di Pisa
White Dwarfs and Fundamental Physics: P. G. Prada Moroni | PDF | Stars | Gases
Theoretical uncertainties on classical Cepheid pulsational quantities
Mixing-Length Estimates From Binary Systems. A Theoretical Investigation on the Estimation Errors
Appunti Fisica
Cumulative theoretical uncertainties in lithium depletion boundary age
Galactic structure and white dwarf populations
Package 'stellaR'
Pre-Main Sequence evolutionary models (low and intermediate mass) Scilla Degl'Innocenti Emanuele Tognelli Pier Giorgio Prada Moroni (Physics Department, - ppt download
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Pre-Main Sequence evolutionary models (low and intermediate mass) Scilla Degl'Innocenti Emanuele Tognelli Pier Giorgio Prada Moroni (Physics Department, - ppt download
Pier Giorgio PRADA MORONI | Associate professor | Ph. D. in Physics | Università di Pisa, Pisa | UNIPI | Department of Physics "E.Fermi"
7Li surface abundance in pre-main sequence stars
Pier Giorgio PRADA MORONI | Associate professor | Ph. D. in Physics | Università di Pisa, Pisa | UNIPI | Department of Physics "E.Fermi"
Consortium Members
2018 Spring Symposia - April 23-26 - Booklet
Mixing-length calibration from field stars - An investigation on statistical errors, systematic biases, and spurious metallicity
arXiv:1510.02620v1 [astro-ph.SR] 9 Oct 2015
Pier Giorgio PRADA MORONI | Associate professor | Ph. D. in Physics | Università di Pisa, Pisa | UNIPI | Department of Physics "E.Fermi"
arXiv:astro-ph/0405101v1 6 May 2004
Frontiers | Theoretical Predictions of Surface Light Element Abundances in Protostellar and Pre-Main Sequence Phase
Stellar models and Hyades: the <i>Hipparcos</i> test
Pisa Stellar Models
The Pisa pre-‐MS tracks and isochrones
