PPT - Pre-Main Sequence evolutionary models (low and intermediate mass) PowerPoint Presentation - ID:2114492
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This Is What Happens When a Star Devours a Planet
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
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
Cieli su Tavolaia - Blog di astronomia » Cielo del mese
Pier Giorgio PRADA MORONI | Associate professor | Ph. D. in Physics | Università di Pisa, Pisa | UNIPI | Department of Physics "E.Fermi"
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
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Iniziativa specifica TAsP (Theoretical Astroparticle Physics)
Pier Giorgio PRADA MORONI | Associate professor | Ph. D. in Physics | Università di Pisa, Pisa | UNIPI | Department of Physics "E.Fermi"
Pier Giorgio Prada Moroni
Quando una stella "mangia" un pianeta | Attualità Pisa
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This Is What Happens When a Star Devours a Planet
Pier Giorgio PRADA MORONI | Associate professor | Ph. D. in Physics | Università di Pisa, Pisa | UNIPI | Department of Physics "E.Fermi"
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When the tale comes true: multiple populations and wide binaries in the Orion Nebula Cluster
