Phd in Physics

Chemo-dynamical evolution of the Milky Way

Chemo-dynamical evolution of the Milky Way

Academic year 2023/2024

Sommario del corso

• Program
• Notes
• Further information
• Class schedule
• Teaching tools
• Course card

Program

• Structure, kinematics, and chemical properties of the Galactic stellar populations (disks, bulge, halo)
• Non axi-symmetric components: bar, spiral arms, flare, warp
• The hierarchical CDM galactic formation scenario
• Elements of Galactic dynamics and cosmological simulations of Milky Way-like disk galaxies
• Wide field stellar surveys (Gaia, RAVE, APOGEE, GES)
• Local cosmology: chemo-dynamical signatures of the Galactic formation processes

Notes

The lectures will take place in January and February 2024. 

Students wishing to take this course must register with the teacher via email  (alessandro.spagna@inaf.it)

Further information

Class schedule

• Teaching material
• Exams and finals
• Class schedule
• Go to Moodle
• Register for the course
• Enrolled students
• Invia email agli studenti registrati
• Export table