Padova 2020 - Multiple Stellar Populations in the next decade CONFERENCE UPDATE 2021 - We regret to inform you that the actual evolution of the pandemic and the consequent situation of the uncertainty at international level oblige us to reschedule to a later date the conference "Padova 2020", upcoming in September 2021. We will keep informing you about possible new dates for this event.

1 Sept 2021, 09:00 → 30 Sept 2021, 16:00 Europe/Rome

Palazzo Santo Stefano

Alessandra Mastrobuono Battisti (Lund University), Amanda Karakas (Monash University), Anna Fabiola Marino (University of Padua), Antonino Milone (University of Padova), Corinne Charbonnel (Geneva Observatory), Edoardo Lagioia (University of Padova), Gary Da Costa (Australian National University), Marco Tailo (University of Padova), Michela Mapelli (University of Padova)

The discovery of multiple stellar populations in globular clusters (GCs) represents one of the most important results of the research in the field of stellar astrophysics. The last two decades witnessed a growing number of studies which, by reversing our vision of simple stellar systems compatible with an isochrone, unveiled the complex nature of the GCs . High-precision photometry color-magnitude diagrams revealed that GCs are composed of two or more discrete stellar groups with specific chemical compositions: one with abundances typical of halo field stars, the other(s) with enhanced light-elements as nitrogen and sodium. A sub-group of clusters also exhibits variations in heavy-elements and iron. 

Several scenarios of formation and evolution of multiple stellar populations have been proposed so far but none of them fulfills at once all the numerous observational constraints. Important questions, therefore, are still open: How did GCs form in the early Universe? What is their role in the assembly of the Galaxy? Did they significantly contribute to the reionization of the Universe?

The aim of this conference is to connect observation and theory to review the state-of-the-art on multiple populations in GCs and discuss the developments of GC studies in the next future.

The main topics include:

• Composition, kinematics, and general properties of multiple populations
• Connection between multiple populations and GC host galaxies
• Models of formation and evolution of multiple populations
• Multiple stellar population in young and open clusters