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
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Pier Giorgio PRADA MORONI | Associate professor | Ph. D. in Physics | Università di Pisa, Pisa | UNIPI | Department of Physics "E.Fermi"
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
Pisa pre-MS models A rich database covering a large range of Z, Y, mass and age values
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"
When the tale comes true: multiple populations and wide binaries in the Orion Nebula Cluster
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Iniziativa specifica TAsP (Theoretical Astroparticle Physics)
CALIBRATION OF WHITE DWARF COOLING SEQUENCES: THEORETICAL UNCERTAINTY Pier Giorgio Prada Moroni and Oscar Straniero ABSTRACT Whi
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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"
Todd Bartel 85 PT | RISD Alumni
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PPT - Pre-Main Sequence evolutionary models (low and intermediate mass) PowerPoint Presentation - ID:2114492
This Is What Happens When a Star Devours a Planet
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
arXiv:2004.14857v1 [astro-ph.SR] 30 Apr 2020
