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Cumulative theoretical uncertainties in lithium depletion boundary age
Cumulative theoretical uncertainties in lithium depletion boundary age

Pre-Main Sequence evolutionary models (low and intermediate mass) Scilla  Degl'Innocenti Emanuele Tognelli Pier Giorgio Prada Moroni (Physics  Department, - ppt download
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
Pier Giorgio PRADA MORONI | Associate professor | Ph. D. in Physics | Università di Pisa, Pisa | UNIPI | Department of Physics "E.Fermi"

Stellar models and Hyades: the <i>Hipparcos</i> test
Stellar models and Hyades: the Hipparcos test

Pre-Main Sequence evolutionary models (low and intermediate mass) Scilla  Degl'Innocenti Emanuele Tognelli Pier Giorgio Prada Moroni (Physics  Department, - ppt download
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
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
arXiv:astro-ph/0702405v1 15 Feb 2007

arXiv:1510.02620v1 [astro-ph.SR] 9 Oct 2015
arXiv:1510.02620v1 [astro-ph.SR] 9 Oct 2015

Asteroseismic age estimates of RGB stars in open clusters - A statistical  investigation of different estimation methods
Asteroseismic age estimates of RGB stars in open clusters - A statistical investigation of different estimation methods

2018 Spring Symposia - April 23-26 - Booklet
2018 Spring Symposia - April 23-26 - Booklet

PDF) Recovering the star formation rate in the solar neighborhood | S.  Degl'Innocenti - Academia.edu
PDF) Recovering the star formation rate in the solar neighborhood | S. Degl'Innocenti - Academia.edu

Theoretical uncertainties on white dwarf luminosity functions
Theoretical uncertainties on white dwarf luminosity functions

Consortium Members
Consortium Members

arXiv:1405.7486v1 [astro-ph.SR] 29 May 2014
arXiv:1405.7486v1 [astro-ph.SR] 29 May 2014

Pier Giorgio PRADA MORONI | Associate professor | Ph. D. in Physics |  Università di Pisa, Pisa | UNIPI | Department of Physics
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
arXiv:astro-ph/0405101v1 6 May 2004

The Pisa pre-‐MS tracks and isochrones
The Pisa pre-‐MS tracks and isochrones

Galactic structure and white dwarf populations
Galactic structure and white dwarf populations

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michele.jpg

Theoretical uncertainties on classical Cepheid pulsational quantities
Theoretical uncertainties on classical Cepheid pulsational quantities

Appunti Fisica
Appunti Fisica

Mixing-length calibration from field stars - An investigation on  statistical errors, systematic biases, and spurious metallicity
Mixing-length calibration from field stars - An investigation on statistical errors, systematic biases, and spurious metallicity

7Li in young open clusters and binary systems
7Li in young open clusters and binary systems

Pisa Stellar Models
Pisa Stellar Models