Code: | AST4001 | Acronym: | AST4001 |
Keywords | |
---|---|
Classification | Keyword |
OFICIAL | Astronomy |
Active? | Yes |
Responsible unit: | Department of Physics and Astronomy |
Course/CS Responsible: | Master in Astronomy and Astrophysics |
Acronym | No. of Students | Study Plan | Curricular Years | Credits UCN | Credits ECTS | Contact hours | Total Time |
---|---|---|---|---|---|---|---|
M:A_ASTR | 12 | Study plan since academic year 2023/2024 | 1 | - | 6 | 42 | 162 |
2 |
The aim of this course is that students acquire a thorough knowledge about different types of galaxies, their composition and the physical mechanisms responsible for the variety of observed properties and their evolution in different environments. Alongside the theoretical approach, existing observational evidence will be presented, and the major ongoing and future projects with scientific impact in this area will be mentioned.
It is intended that students acquire a thorough knowledge about different types of galaxies, their composition and the physical mechanisms responsible for the variety of observed properties and their evolution in different environments. Alongside the theoretical approach, it is expected that students develop skills of reasoning and understanding, critical analysis and exposition of different results available in the literature and, if possible, experience a brief approach to research in this topic through the small project that is proposed.
I. The Milky Way - structure, dimensions, main constituents (stars, interstellar medium, dark matter).
II. Galaxy classification schemes and main properties of the different galaxy types.
III. Disks and spheroids - dynamics, total mass estimates, scaling relations and statistical properties. Star formation in disks.
IV. Spectral synthesis: main types, ingredients and equations.
V. Groups and clusters of galaxies: dimensions, constituents and main properties.
VI. Physical mechanisms responsible for galactic evolution in groups and clusters: dynamical friction, ram-pressure stripping, tidal stripping, mergers.
VII. Active galaxy nuclei - emission; different types of AGN and the unification scheme. Estimates of the mass of the central supermassive black hole.
VIII. High redshift galaxies and evolutionary studies: techniques and types of distant galaxies; K and E corrections; observational biases; evolution in color, morphology, star formation rate and stellar mass function.
Throughout the semester, references for scientific papers dealing with the subjects taught will be provided.
The classes consist of an exposition of the contents of the syllabus, with the help of multimedia. The aim is also to create moments for discussion of concepts or scientific results based on relevant and/or recent articles, in order to promote active learning. Exercises are also solved when appropriate.
designation | Weight (%) |
---|---|
Exame | 50,00 |
Participação presencial | 5,00 |
Apresentação/discussão de um trabalho científico | 25,00 |
Trabalho prático ou de projeto | 20,00 |
Total: | 100,00 |
designation | Time (hours) |
---|---|
Estudo autónomo | 60,00 |
Frequência das aulas | 42,00 |
Trabalho laboratorial | 30,00 |
Apresentação/discussão de um trabalho científico | 30,00 |
Total: | 162,00 |
Assessment in the course consists of:
1) 50% - final written exam, with consultation - compulsory (in normal or appeal period) and with a minimum mark of 8/20;
and the following Distributed Assessment components:
2) 5% - participation in class discussions prompted by questions posed by the teacher;
3) 45% - practical work with a report (20%) and (partial) presentation and oral discussion (25%).
The practical computer work is carried out throughout the semester under the supervision of the teachers. The written report is due on the last day of the course, where the results will also be presented and discussed.
The improvement of the classification can be made on the written exam component only, that will still weigh 50% of the final mark.