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Uncertainties in stellar ages provided by grid techniques
Uncertainties in stellar ages provided by grid techniques

Package 'stellaR'
Package 'stellaR'

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

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

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giovanni.jpg

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michele.jpg

Pier Giorgio PRADA MORONI | Associate professor | Ph. D. in Physics |  Università di Pisa, Pisa | UNIPI | Department of Physics "E.Fermi"
Pier Giorgio PRADA MORONI | Associate professor | Ph. D. in Physics | Università di Pisa, Pisa | UNIPI | Department of Physics "E.Fermi"

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

Appunti Fisica
Appunti Fisica

Effect of planet ingestion on low-mass stars evolution: The case of 2MASS  J08095427-4721419 star in the Gamma Velorum cluster
Effect of planet ingestion on low-mass stars evolution: The case of 2MASS J08095427-4721419 star in the Gamma Velorum cluster

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

Pier Giorgio PRADA MORONI | Associate professor | Ph. D. in Physics |  Università di Pisa, Pisa | UNIPI | Department of Physics "E.Fermi"
Pier Giorgio PRADA MORONI | Associate professor | Ph. D. in Physics | Università di Pisa, Pisa | UNIPI | Department of Physics "E.Fermi"

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 "E.Fermi"
Pier Giorgio PRADA MORONI | Associate professor | Ph. D. in Physics | Università di Pisa, Pisa | UNIPI | Department of Physics "E.Fermi"

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

Pier Giorgio PRADA MORONI | Associate professor | Ph. D. in Physics |  Università di Pisa, Pisa | UNIPI | Department of Physics "E.Fermi"
Pier Giorgio PRADA MORONI | Associate professor | Ph. D. in Physics | Università di Pisa, Pisa | UNIPI | Department of Physics "E.Fermi"

Pier Giorgio PRADA MORONI | Associate professor | Ph. D. in Physics |  Università di Pisa, Pisa | UNIPI | Department of Physics "E.Fermi"
Pier Giorgio PRADA MORONI | Associate professor | Ph. D. in Physics | Università di Pisa, Pisa | UNIPI | Department of Physics "E.Fermi"

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

Scoperta una nuova classe di stelle all'Università di Pisa
Scoperta una nuova classe di stelle all'Università di Pisa

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

Frontiers | Theoretical Predictions of Surface Light Element Abundances in  Protostellar and Pre-Main Sequence Phase
Frontiers | Theoretical Predictions of Surface Light Element Abundances in Protostellar and Pre-Main Sequence Phase

Mixing-Length Estimates From Binary Systems. A Theoretical Investigation on  the Estimation Errors
Mixing-Length Estimates From Binary Systems. A Theoretical Investigation on the Estimation Errors

arXiv:astro-ph/0702405v1 15 Feb 2007
arXiv:astro-ph/0702405v1 15 Feb 2007

7Li surface abundance in pre-main sequence stars
7Li surface abundance in pre-main sequence stars