Pisa pre-MS models A rich database covering a large range of Z, Y, mass and age values
CALIBRATION OF WHITE DWARF COOLING SEQUENCES: THEORETICAL UNCERTAINTY Pier Giorgio Prada Moroni and Oscar Straniero ABSTRACT Whi
This Is What Happens When a Star Devours a Planet
Pisa pre-MS models A rich database covering a large range of Z, Y, mass and age values
Corso di Laurea: BIO-L Nome del corso: Fisica (Corso B
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 Pisa pre-‐MS tracks and isochrones
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