Consortium Members
Esercizi Fisica
THE EFFECT OF 12 C(α,γ) 16 O ON WHITE DWARF EVOLUTION Pier Giorgio Prada Moroni Dipartimento di Fisica - Università di Pisa Osservatorio Astronomico di. - ppt download
Pier Giorgio PRADA MORONI | Associate professor | Ph. D. in Physics | Università di Pisa, Pisa | UNIPI | Department of Physics "E.Fermi"
The Pisa pre-main sequence stellar evolutionary models: results for non-accreting and accreting models
PPT - Pre-Main Sequence evolutionary models (low and intermediate mass) PowerPoint Presentation - ID:2114492
Pier Giorgio PRADA MORONI | Associate professor | Ph. D. in Physics | Università di Pisa, Pisa | UNIPI | Department of Physics "E.Fermi"
Community Advisory Council | KNKX Public Radio
CALIBRATION OF WHITE DWARF COOLING SEQUENCES: THEORETICAL UNCERTAINTY Pier Giorgio Prada Moroni and Oscar Straniero ABSTRACT Whi
Pisa pre-MS models A rich database covering a large range of Z, Y, mass and age values
When the tale comes true: multiple populations and wide binaries in the Orion Nebula Cluster
Igor Vitale | Facebook
Corso di Laurea: BIO-L Nome del corso: Fisica (Corso B
Quando una stella "mangia" un pianeta | Attualità Pisa
Pier Giorgio PRADA MORONI | Associate professor | Ph. D. in Physics | Università di Pisa, Pisa | UNIPI | Department of Physics "E.Fermi"
Iniziativa specifica TAsP (Theoretical Astroparticle Physics)
Cefalu 2007
Pier Giorgio PRADA MORONI | Associate professor | Ph. D. in Physics | Università di Pisa, Pisa | UNIPI | Department of Physics "E.Fermi"
This Is What Happens When a Star Devours a Planet
Advisory Board | Mysite
Flamingo stars turn pink when they gobble iron-rich planets | New Scientist
