Galaxies: formation and evolution

(tylko po angielsku) 1. knowledge of linear algebra and calculus.

2. basic knowledge of mechanics and thermodynamics.

(tylko po angielsku) Contact hours with teacher:

- participation in lectures - 30 hrs

- participation in tutorials - 30 hrs

Self-study hours:

- preparation for lectures - 30 hrs

- preparation for tutorials –30hrs

- preparation for examination- 30 hrs

Altogether: 150 hrs (5 ECTS)

(tylko po angielsku) Student:

W1 – knows physical processes taking place in galaxies and interstellar medium, knows the structure, dynamics and evolution of galaxies. (K_W04)

W2 – knows the role of theoretical methods and numerical simulations in the research on galactic dynamics and evolution. (K_W03)

W3 – knows modern trends in studies of galactic evolution. (K_W06)

(tylko po angielsku) Student:

U1: is able to use mathematical apparatus and numerical experiments in modeling the dynamics of stars and interstellar medium of galaxies. (K_U02)

U2: Can use and modify available software for numerical modeling fluid-dynamical phenomena in astrophysics. (K_U04)

(tylko po angielsku) Student

K1: understands the importance and limitation of mathematical and numerical modeling in investigations of complex dynamical and evolutionary processes in galaxies. (K_K01)

(tylko po angielsku) Lectures: Expository teaching methods - informative lecture.

Tutorials: Exploratory teaching methods - computer laboratory for experimenting with numerical models of galaxies.

- symulacyjna (gier symulacyjnych)

- wykład informacyjny (konwencjonalny)

- laboratoryjna

- gry i symulacje
- metody służące prezentacji treści