Resolved stellar populations
Leaders
Sebastian Kamann
John Moores University Liverpool, United Kingdom
Anna McLeod
Durham University, United Kingdom
Martin M. Roth
Leibniz-Institut für Astrophysik Potsdam, Germany
Sub-working groups & co-leaders
Origins of the elements: neutron capture elements
Tadafumi Matsuno · Nick Storm · Valeria Grisoni
Origins of the elements: SN Ia
Chiaki Kobayashi · Federico Sestito · Anish Amarsi
Origins of the MW system - Hierarchical formation and ex-situ populations
Nicolas Martin · Salvatore Taibi · Anke Arden-Arentsen
Origins of the MW system - In-situ populations and the disc + Bulge connection
Maria Bergemann · Georges Kordopatis
Origins of stars and planets - characterization of planet-host stars and environmental dependence of planet formation
Maria Tsantaki · Katia Biazzo
Origins of stars and planets - star formation and young stellar populations
Germano Sacco · Carlo Manara
The dynamic Universe
Black holes growth across time and mass
Galaxy assembly across physical scale
Star and planet formation
Stars, their end points, feedback, and elements production
New frontiers in cosmology
Related pages
Main section
Science team
The Science Team plays a key role in proposing and developing transformative science cases and in shaping the science-driven requirements for the WST.
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