Sfoglia per Relatore
Mostrati risultati da 1 a 19 di 19
Binaries among multiple populations in the globular cluster 47 Tucanae
2023/2024 BERNIZZONI, MARA
Caratterizzazione delle nubi primordiali tramite le stelle di prima popolazione degli ammassi globulari
2023/2024 GHIRALDO, VALENTINA
Helium and multiple stellar populations in the massive outer-halo globular cluster NGC 2419.
2019/2020 Zennaro, Marco
HST photometry of multiple populations in the type II globular cluster NGC 6273
2022/2023 ZERAJIC DE GIORGIO, MARIANNA
Hunting UV-dim stars in Magellanic Cloud star clusters with HST
2022/2023 MURATORE, FABRIZIO
Indagando le stelle di popolazione III
2021/2022 BHATTI, ROBEN
Internal kinematics of stellar populations in M54 and in the Sagittarius dwarf galaxy.
2021/2022 Martorano, Marco
Internal kinematics of stellar populations in M54 and in the Sagittarius dwarf galaxy
2020/2021 MARTORANO, MARCO
Internal kinematics of stellar populations in Terzan 5
2021/2022 MAGLIONE, MARIASOLE
Multiple Populations among very low mass stars in 47 Tucanae
2022/2023 BAIMUKHAMETOVA, SARAH
Multiple populations among very low-mass stars in NGC288
2021/2022 BORTOLAN, EMANUELE
Nubi primordiali e formazione degli ammassi globulari
2022/2023 PUGGIONI, DARIO
Photometry and astrometry of M22: an integration with spectroscopy for a state-of-the-art characterization.
2023/2024 BOURAS MORENO SANCHEZ, AUGUSTO
Photometry and proper motions of Milky-Way satellites with the Hubble Space Telescope
2021/2022 TROIA, ANDREA
Sistemi stellari massivi: determinazione dei parametri astrofisici fondamentali di HD114886A
2023/2024 SCHENONE ZANUZZI, ANTONELLA
Smoldering Embers - The Search for Slowly Cooling White Dwarfs in Globular Clusters NGC0288 and NGC0362
2023/2024 LIONETTO, SOFIA
Spectral analysis of the multiple populations in Omega Centauri with MUSE
2022/2023 DI STEFANO, SIMONA
Stelle di massa molto ridotta negli ammassi globulari
2022/2023 POSENATO, MICHELA
The non-LTE copper abundance of the Sun
2022/2023 RACCA, MILA
Mostrati risultati da 1 a 19 di 19
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