When the tale comes true: multiple populations and wide binaries in the Orion Nebula Cluster
Pier Giorgio PRADA MORONI | Associate professor | Ph. D. in Physics | Università di Pisa, Pisa | UNIPI | Department of Physics "E.Fermi"
Cefalu 2007
Igor Vitale | Facebook
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The Pisa pre-‐MS tracks and isochrones
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
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Pier Giorgio Prada Moroni
Todd Bartel 85 PT | RISD Alumni
Pisa pre-MS models A rich database covering a large range of Z, Y, mass and age values
This Is What Happens When a Star Devours a Planet
The Pisa pre-main sequence stellar evolutionary models: results for non-accreting and accreting models
Cefalu 2007
Corso di Laurea: BIO-L Nome del corso: Fisica (Corso B
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arXiv:2004.14857v1 [astro-ph.SR] 30 Apr 2020
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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"
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"
