Calendar

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Seminario: presentazione della tesi di Marco Tarantino (UNIPA), Aula ore 12 12:00
Seminario: presentazione della tesi di Marco Tarantino (UNIPA), Aula ore 12
Ott 4@12:00–13:30
Speaker: Marco Tarantino Studente Magistrale in Statistica e Data Science (LM-82), Universita’  degli Studi di Palermo Titolo: APPLICAZIONE DI TECNICHE STATISTICHE PER LA PREVISIONE DELLA TEMPERATURA EFFETTIVA DI STELLE GIOVANI Abstract: Uno degli attuali argomenti di discussione riguarda la durata del processo di formazione di cluster stellari: vi sono modelli teorici che ipotizzano un unico evento dal quale si formano tutte
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Seminario: presentazione Tesi G. La Malfa (UNIPA) 15:00
Seminario: presentazione Tesi G. La Malfa (UNIPA)
Ott 5@15:00–16:30
Speaker: Giorgio La Malfa Relatore: Marco Miceli Titolo:Anisotropies in core-collapse supernova explosions: modeling the evolution of a magnetorotational supernova remnant Abstract: The core-collapse supernovae (CCSNe) whose explosion is driven by mag- netorotational instabilities (MRIs) are believed to be viable sources of extremely interesting astrophysical phenomena, such as hypernovae, super-luminous SNe, magnetars and gamma-ray bursts. Observations of the supernova remnants (SNRs)
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Seminario: Mario Guarcello (INAF), ore 15 15:00
Seminario: Mario Guarcello (INAF), ore 15
Ott 12@15:00–16:30
Speaker: Mario Guarcello (INAF) Titolo: “EWOCS: status of the project.” Abstract: “The EWOCS project has the objective of studying star and planet formation, and early stellar evolution, in very young massive clusters (VYMCs). With a mass in excess of 10^4 solar masses, the very few VYMCs known in the Milky Way represent the most accessible examples of starburst regions, which
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Seminario: Maria Kopsacheili (ICE-CSIC), Aula ore 15 15:00
Seminario: Maria Kopsacheili (ICE-CSIC), Aula ore 15
Ott 18@15:00–16:30
Speaker: Maria Kopsacheili (ICE-CSIC) Titolo: New larger sample of Supernova Remnants in NGC 7793, using MUSE IFS. Abstract: Study of Supernova Remnant (SNR) demographics and their physical properties (density, temperature, shock velocities) is very important in order to understand their role in galaxies. Many photometric and spectroscopic studies of SNRs have been carried out in our Galaxy but also in
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