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Chemo-dynamical evolution of the Milky Way

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14-Chemo-dynamical evolution of the Milky Way

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Academic year 2021/2022

Teacher
Alessandro Spagna
Degree course
PhD in Physics
Teaching period
First semester
Credits/Recognition
2
Course disciplinary sector (SSD)
FIS/05 - astronomy and astrophysics
Delivery
Formal authority
Language
English
Attendance
Obligatory
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Sommario del corso

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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

Suggested readings and bibliography

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Binney & Merrifield, Galactic Astronomy



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Note

Students wishing to take this course must register with the teacher via email

Period

TBD

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Last update: 27/01/2022 15:57
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