Galaxies

Spiral galaxy NGC 3627 (M66). Credit: ESO/P. Barthel
The focus of the course is on properties of different types of galaxies, but mainly on processes that are especially important for how galaxies evolve: star formation, dynamic processes within and between galaxies, and active galactic nuclei. Subjects such as stellar orbits in galaxies, star formation in galaxies, disk and elliptical galaxies and active galactic nuclei will be covered.
After taking the course you are expected to have acquired advanced knowledge on galaxies and the underlying astrophysical processes that govern their formation and evolution. Specifically, you should be able to:
- describe different types of galaxies, and the astrophysical processes that give rise to the observable properties of them
- qualitatively describe star formation in galaxies, galaxy dynamics, chemical enrichment in galaxies, and the electromagnetic spectrum of galaxies
- solve calculation problems relating to star formation in galaxies, galaxy dynamics, chemical enrichment in galaxies, and the electromagnetic spectrum of galaxies
- show understanding for how galaxies are affected, quantitatively and qualitatively, as they evolve and interact
- show good insight in, and understanding of, modern extragalactic research, as well as discuss this at seminars.
The course is given during day time, and is part of the Master’s programme in Astronomy. It can also be taken as a free-standing course. The course is given in English.
Teaching Format
The course consistss of interactive lectures and seminars. The seminars are compulsory.
Assessment
To pass the course you need to have attended both seminar sessions. There are multiple choice tests and a written exam.
Examiner
Matthew Hayes
Cimatti, Fraternali, & Nipoti: “Introduction to Galaxy Formation and Evolution”, 2020, Cambridge University Press.





