Chemical and dynamical evolution of the Milky Way and Local Group galaxies | ||
Each contribution consists of a 30 min talk plus 15 min for discussion | ||
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18 January | ||
18:00 19:30 PM | Registration and Welcome Party | |
19 January Session 1 Milky Way Disk(s) | ||
8:30 9:15 AM | Galactocentric variation of the abundance structure in the Milky Way stellar disk - results from the Gaia-ESO survey (N.A.) | Bensby |
9:15-10:00 AM | Stellar abundances in clusters | Bragaglia |
10:00 10:45 AM | Tracing chemical evolution over the extent of the Milky Way's Disk with APOGEE Red Giant Stars | Nidever |
11:30 am -4:00 pm | Lunch and ski break | |
4:00 4:30 PM | Coffee Break | |
4:30 5:15 PM | The formation and evolution of the galactic disks | Haywood |
5:15 6:00 PM | The Imprints of Disk Evolution on the Vertical Structure of the Milky Way Disk | Schlesinger |
6:00 6:45 PM | Abundance gradient across the thin Galactic disk (N.A.) | Bono |
08:30:00 PM | FIACCOLATA walk (free) | |
a nice 20 min walk with torches to a rifugio where we will have fun | ||
20 January -Session 2 - Milky Way Thick Disk and Bulge | ||
8:30 9:15 AM | Composition and Kinematics of the Bulge | Rich |
9:15 10:00 AM | RR Lyrae in the Galactic Bulge. VVV Vista Variables in the Via Lactea | Minniti |
10:00 10:45 AM | Detailed near-IR stellar abundances of red giants in the Bulge | Ryde |
10:45 11:30 AM | The Galactic Bulge and Bar | Gerhard |
11:30 AM -4:00 PM | Lunch and ski break | |
4:00 4:30 PM | Coffee Break | |
4:30 5:15 PM | On the connection between the galactic disk and the galactic bar | Spagna |
5:15 6:00 PM | The promise of the Open Clusters in the Gaia-ESO Survey | Magrini |
20 January Session 3 - Milky Way Thick Disk and Halo | ||
6:00 6:45 PM | Modeling the Milky Way: the thick disc, the bulge, and the outer Galactic disc | Di Matteo |
21 January Session 3 - Continuation | ||
8:30 9:15 AM | Spectroscopic characterization on Globular Clusters multiple populations (N.A.) | Lucatello |
9:15 10:00 AM | The early life of Globular Clusters. Chemistry and dynamics Evolution | Charbonnel |
10:00 10:45 AM | First stars and their local relics | Schneider |
10:45 - 11:30 AM | Understanding the formation of the Milky Way in the era of Gaia | Minchev |
11:30 AM - 4 PM | Lunch and sky break | |
21 January Session 4 - Stellar Evolution and Ages | ||
4:00 4:30 PM | Coffee Break | |
4:30 5:15 PM | Presupernova evolution and nucleosyntesis of rotating massive stars at various metallicities | Limongi |
5:15 6:00 PM | Cumulative theoretical uncertainties in Lithium depletion boundary age | Tognelli |
6:00 6:45 PM | SFR history and bayesian ages of MW stars | Morossi |
22 January Session 5 - Local Group Galaxies | ||
8:30 9:15 AM | Stellar models, globular and open clusters, and satellite dwarfs:all are tracers of the chemical and dynamical evolution of the MW and LG galaxies | Tosi |
9:15 10:00 AM | The PN population in the MW, Local Group and beyond | Arnaboldi |
10:00 10:45 AM | The chemical evolution of the smallest Milky Way satellites: Bootes I | Romano |
10:45 11:30 AM | RR Lyrae stars: building-up the Galactic halo with dwarf spheroidals | Fiorentino |
11:30 am -4:00 pm | Lunch and ski break | |
22 January Session 6 - Chemo-dynamical Models and Star Formation | ||
4:00 4:30 PM | Coffee Break | |
4:30 5:15 PM | The effect of stellar migration on Galactic chemical evolution: a heuristic approach | Spitoni |
5:15 6:00 PM | The chemical evolution of Sagittarius: the effect of different IMFs | Vincenzo |
6:00 6:45 PM | Chemical Composition of Local Group Dwarf Galaxies and Chemical Evolution | Mcwilliam |
6:45 7:00 PM | Nitrogen in Damped Ly-α Galaxies | Molaro |
08:00 PM | Social dinner at Bad-mos Hotel (for people with no half-board at the hotel there is an extra cost) | |
23 January Session 6 - Continuation | ||
8:30 9:15 AM | A new method to compute the chemical enrichment from multiple stellar populations | Calura |
9:15 10:00 AM | Stellar dynamics and radial gas flows in disk galaxies | Ciotti |
10:00 10:45 AM | The structure of molecular clouds and their influence on star formation | Lombardi |
10:45 11:30 AM | Molecular clouds properties in galactic scale simulations | Khoperskov |
11:30 11:45 AM | Galactic Evolution of Eu: NSM vs. Sne | Matteucci |