Advisory Board | Mysite
People | Marine Futures
Pier Giorgio PRADA MORONI | Associate professor | Ph. D. in Physics | Università di Pisa, Pisa | UNIPI | Department of Physics "E.Fermi"
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Iniziativa specifica TAsP (Theoretical Astroparticle Physics)
The Pisa pre-main sequence stellar evolutionary models: results for non-accreting and accreting models
Pier Giorgio PRADA MORONI | Associate professor | Ph. D. in Physics | Università di Pisa, Pisa | UNIPI | Department of Physics "E.Fermi"
PPT - Pre-Main Sequence evolutionary models (low and intermediate mass) PowerPoint Presentation - ID:2114492
Todd Bartel 85 PT | RISD Alumni
Pisa pre-MS models A rich database covering a large range of Z, Y, mass and age values
Esercizi Fisica
Pier Giorgio Prada Moroni
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
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
Cefalu 2007
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Quando una stella "mangia" un pianeta | Attualità Pisa
The Pisa pre-‐MS tracks and isochrones
This Is What Happens When a Star Devours a Planet
This Is What Happens When a Star Devours a Planet
When the tale comes true: multiple populations and wide binaries in the Orion Nebula Cluster
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