The Milky Way Assembly Tale - Plot and characters as of today, and what to expect in future editions

Europe/Rome
Bologna

Bologna

Via Piero Gobetti, 101, 40129 Bologna BO
Description
 
Our knowledge of the Milky Way's assembly history has been revolutionised by the advent of the Gaia mission. Since the availability of kinematic information for more than 1 billion stars with Gaia DR2, the story of how our Galaxy was formed from the merger of smaller galaxies has begun to unravel. Gaia's handwriting has been supported by the combination of its dynamical information with chemical abundance and age measurements from spectroscopic (e.g. APOGEE, GALAH, GES, LAMOST, RAVE) and asteroseismic (e.g. CoRoT, Kepler, K2, TESS) surveys, which are now adding more detail to the plot. However, as the plot unravels, it becomes more and more complex. Observations and models need to move forward in tandem to support its evolution and uncover possible twists. Future large-scale spectroscopic surveys will greatly improve our chemical knowledge of the Milky Way's stellar populations and, together with future asteroseismic missions, will open the window to systematic determination of accurate stellar ages as a new ink to fuel the writing.
 
With the rapid pace at which the Milky Way assembly story is constantly being updated, the aim of this conference is to bring the community onto the same page, where the main characters, their characteristics and the timeline of their contribution are well established, and where the main observational and theoretical open questions for the continuation of the story are set out and discussed.

 
The topics to be covered at the conference are as follows
 
  • Substructures of the Milky Way halo, in the chemical-dynamical-chronological space;
     
  • Evolution of the Milky Way disk through the interplay with the assembling mergers;
     
  • Stellar age as a critical component - development of new methods to infer age with increased precision and accuracy and cosmological implications;
     
  • Predictions from simulations as a tool for interpreting the complex observational evidence;
     
  • The assembly history of the Local Group.

 

Important information on unsolicited requests for hotels bookings

Please note that the official partner of the "Milky Way Tale Conference" is Planning Congressi srl (https://planning.it/). We urge caution in case you receive unsolicited offers to provide hotel rooms or other services from different companies, or unsolicited phone calls requesting, e.g., to confirm your hotel reservations. We strongly advise you not to contact them or provide them with any of your personal details, and cannot accept any responsibility for adverse consequences should you choose to do so. In case of any questions, please kindly contact Planning at r.suzzi@planning.it.

    • 09:00 10:30
      Session: MW Halo chemo-dynamics
      • 09:00
        A. Helmi (Invited) 30m
      • 09:30
        L. Thulasidharan 20m
      • 09:50
        A. Viswanathan 20m
      • 10:10
        E. Ceccarelli 20m
    • 10:30 11:00
      Coffee Break 30m
    • 11:00 12:30
      Session: MW Halo chemo-dynamics
      • 11:00
        V. Belokurov (Invited) 30m
      • 11:30
        A. Dillamore 20m
      • 11:50
        J. Nibauer 20m
      • 12:10
        V. Chandra 20m
    • 12:30 14:00
      Lunch Break 1h 30m
    • 14:00 15:30
      Session: MW Halo chemo-dynamics
      • 14:00
        D. Feuillet (Invited) 30m
      • 14:30
        D. Aguado 20m
      • 14:50
        B. Chen 20m
      • 15:10
        T. Matsuno 20m
    • 15:30 16:00
      Coffe Break 30m
    • 16:00 18:00
      Session: MW Halo chemo-dynamics
      • 16:00
        E. Starkenburg (Invited) 30m
      • 16:30
        A. Arentsen 20m
      • 16:50
        A. Mori 20m
      • 17:10
        S. Buder 20m
      • 17:30
        Discussion 30m
    • 09:00 10:30
      Session: MW Halo chemo-dynamics
      • 09:00
        H. W. Rix (Invited) 30m
      • 09:30
        D. Horta 20m
      • 09:50
        S. Monty 20m
      • 10:10
        S. Pearson 20m
    • 10:30 11:00
      Coffe Break 30m
    • 11:00 12:30
      Session: MW Halo chemo-dynamics
      • 11:00
        E. Cunningham (Invited) 30m
      • 11:30
        S. Taibi 20m
      • 11:50
        F. Hammer 20m
      • 12:10
        E. Fernandez-Alvar 20m
    • 12:30 14:00
      Lunch Break 1h 30m
    • 14:00 15:30
      Session: MW Disc chemo-dynamics
      • 14:00
        C. Chiappini (Invited) 30m
      • 14:30
        N. Pranzos 20m
      • 14:50
        H. Zhang 20m
      • 15:10
        L. Marques 20m
    • 15:30 16:00
      Coffe Break 30m
    • 16:00 18:00
      Session: MW Disc chemo-dynamics
      • 16:00
        C. Laporte (Invited) 30m
      • 16:30
        P. McMillan 20m
      • 16:50
        T. Antoja 20m
      • 17:10
        F. Sestito 20m
      • 17:30
        Discussion 30m
    • 09:00 10:20
      Session: MW Disc chemo-dynamics
      • 09:00
        N. Lagarde 20m
      • 09:20
        A. Queiroz 20m
      • 09:40
        M. del Alcazar Julia 20m
      • 10:00
        N. Cambiaso 20m
    • 10:20 10:50
      Coffe Break 30m
    • 10:50 12:20
      Session: MW Disc chemo-dynamics
      • 10:50
        A. Recio-Blanco (Invited) 30m
      • 11:20
        K. Hawkins 20m
      • 11:40
        B. Radcliffe 20m
      • 12:00
        Nataf 20m
    • 12:20 13:50
      Lunch Break 1h 30m
    • 13:50 15:20
      Session: Extra-galactic assembly
      • 13:50
        A. Mucciarelli (Invited) 30m
      • 14:20
        E. Vasiliev 20m
      • 14:40
        M. Pawlowski 20m
      • 15:00
        E. Davies 20m
    • 15:20 15:50
      Coffe Break 30m
    • 15:50 17:50
      Session: Extra-galactic assembly
      • 15:50
        A. Ferguson (Invited) 30m
      • 16:20
        C. Tsakonas 20m
      • 16:40
        I. Escalla 20m
      • 17:00
        M. Bellazzini 20m
      • 17:20
        Discussion 30m
    • 19:30 22:30
      Social dinner: SOCIAL DINNER : CANTINA BENTIVOGLIO, VIA MASCARELLA 4/B, 40126 BOLOGNA [ indicative start time: 19:30 ]
    • 09:00 10:30
      Session: Heavy data
      • 09:00
        G. Guiglion (Invited) 30m
      • 09:30
        G. Thomas 20m
      • 09:50
        S. Nepal 20m
      • 10:10
        A. Sante 20m
    • 10:30 11:00
      Coffe Break 30m
    • 11:00 12:40
      Session: The role of age
      • 11:00
        P. Das (Invited) 30m
      • 11:30
        C. Gallart (Invited) 30m
      • 12:00
        M. Cignoni 20m
      • 12:20
        L. Casamiquela 20m
    • 12:40 14:10
      Lunch Break 1h 30m
    • 14:10 15:40
      Session: The role of age
      • 14:10
        K. Brogaard (Invited) 30m
      • 14:40
        M. Monelli 20m
      • 15:00
        P. Moroni 20m
      • 15:20
        G. Buldgen 20m
    • 15:40 16:10
      Coffe Break 30m
    • 16:10 18:10
      Session: The role of age
      • 16:10
        G. Meynet (Invited) 30m
      • 16:40
        G. Casali 20m
      • 17:00
        J. Montalbán 20m
      • 17:20
        S. Hekker 20m
      • 17:40
        Discussion 30m
    • 09:00 10:30
      Session: Predictions by simulations
      • 09:00
        T. Buck (Invited) 30m
      • 09:30
        A. Beane 20m
      • 09:50
        A. Wetzel 20m
      • 10:10
        J. Amarante 20m
    • 10:30 11:00
      Coffe Break 30m
    • 11:00 12:30
      Session: Predictions by simulations
      • 11:00
        R. Grand (Invited) 30m
      • 11:30
        S. Khoperskhov 20m
      • 11:50
        T. Tomlinson 20m
      • 12:10
        E. Wempe 20m
    • 12:30 14:00
      Lunch Break 1h 30m