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Flamingo stars turn pink when they gobble iron-rich planets | New Scientist
The Pisa pre-main sequence stellar evolutionary models: results for non-accreting and accreting models
Pier Giorgio Prada Moroni
This Is What Happens When a Star Devours a Planet
CALIBRATION OF WHITE DWARF COOLING SEQUENCES: THEORETICAL UNCERTAINTY Pier Giorgio Prada Moroni and Oscar Straniero ABSTRACT Whi
Cieli su Tavolaia - Blog di astronomia » Cielo del mese
Loop | Pier Giorgio Prada Moroni
arXiv:2004.14857v1 [astro-ph.SR] 30 Apr 2020
PPT - Pre-Main Sequence evolutionary models (low and intermediate mass) PowerPoint Presentation - ID:2114492
Iniziativa specifica TAsP (Theoretical Astroparticle Physics)
Esercizi Fisica
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"
Untitled
Cefalu 2007
People | Marine Futures
Corso di Laurea: BIO-L Nome del corso: Fisica (Corso B
Appunti Fisica
Pier Giorgio PRADA MORONI | Associate professor | Ph. D. in Physics | Università di Pisa, Pisa | UNIPI | Department of Physics "E.Fermi"
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The Pisa pre-‐MS tracks and isochrones
