Early Formation and Evolution of Bulge and HalO
EFEBHO
Project PRIN MUR 2022 (code 2022ARWP9C - CUP C53D23001000006)
PI: Marconi, M., funded by European Union – Next Generation EU.
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EFEBHO aims to unveil the structure, composition, and origin of the Galactic spheroid (Halo and Bulge) using RR Lyrae stars as reliable beacons of the ancient Milky Way.
EFEBHO aims to unveil the structure, composition, and origin of the Galactic spheroid (Halo and Bulge) using RR Lyrae stars as reliable beacons of the ancient Milky Way.
Research Units
Research Units
INAF - Capodimonte Astronomical Observatory
INAF - Capodimonte Astronomical Observatory
PI Marcella Marconi
Collaborators: Massimo Dall'Ora, Silvio Leccia, Roberto Molinaro, Ilaria Musella, Vincenzo Ripepi
PI Giuseppe Bono
Collaborators:G. Fiorentino, M. Di Criscienzo, Michele Fabrizio,......
UniBo
UniBo
Bologna University
Bologna University
PI Luca Ciotti
Collaborators:
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