Code: | AST602 | Acronym: | AST602 |
Keywords | |
---|---|
Classification | Keyword |
OFICIAL | Astronomy |
Active? | Yes |
Responsible unit: | Department of Physics and Astronomy |
Course/CS Responsible: | Doctoral Program in Astronomy |
Acronym | No. of Students | Study Plan | Curricular Years | Credits UCN | Credits ECTS | Contact hours | Total Time |
---|---|---|---|---|---|---|---|
PDA | 6 | P.E. do Programa Doutoral em Astronomia | 1 | - | 6 | 30 | 162 |
Teacher | Responsibility |
---|---|
Mário João Pires Fernandes Garcia Monteiro |
Theoretical and practical : | 1,15 |
Type | Teacher | Classes | Hour |
---|---|---|---|
Theoretical and practical | Totals | 1 | 1,154 |
Susana Cristina Cabral de Barros | 0,577 | ||
Mário João Pires Fernandes Garcia Monteiro | 0,00 | ||
Ângela Raquel Gonçalves dos Santos | 0,577 |
In this UC the students develop the necessary skills to understand and be prepared for research in advanced topics related to the study of stars and planets. Two topics are chosen annually among a number of possibilities that include studies of: the sun, the solar system, the physics and dynamics of stellar interiors, the evolution of stars, the formation and evolution of exoplanetary systems, the detection and characterization of exoplanets, the astrochemistry of the interstellar medium, astrobiology, among others. At the end of the UC the students must understand and be able to apply techniques that are currently in use by the scientific community working on the selected topics. These can include techniques for the extraction of information from the data, for data interpretation, for the modeling of physical phenomena, etc. Students are also expected to be able to critically review articles related to those topics and to identify associated open questions.
The syllabus ensures that students are exposed to all material required for the full understanding of the topics under consideration. In particular it introduces critical theoretical aspects that are not addressed in previous university stages and tools that allow the students to interpret relevant data. The syllabus also ensures that the student is exposed to recent published results in that research area and acquires a clear perspective of the future evolution of the field.
The contents depend on the topics selected each year, within the area of research on planest and stars. Possible topics for this academic year may be:
B. Stellar magnetic activity:
B1) Solar magnetic activity and rotation
B2) Classification of solar-like stars
B3) Observations for stellar magnetic activity and rotation
B4) Magnetic-activity and angular momentum evolution
B5) Relation between magnetic-activity and rotation
B6) Asteroseismology of magnetic cycles
B7) Magnetism in other types of stars
B8) Open questions and the future
The modules are based in presentations by the lectures (board or video), joint work on specific problems, discussion of research articles, presentations by the students and/or resolution of exercises.
The presentations by the lectures will guarantee that the students gain the necessary background to follow and actively work on the subjects under consideration. These will generally include aspects of the physics of the problem, as well as the details of techniques currently used in the field, and may also introduce currentlyinuse software. The joint work and resolution of exercises will guarantee that the students develop the skills necessary to apply the information, techniques and other material introduced by the lectures to real case studies. The presentation by the students of recent research articles guarantees that they get in close contact to ongoing research related to the topics under consideration at the same time as they develop a critical view on research.
designation | Weight (%) |
---|---|
Prova oral | 50,00 |
Trabalho escrito | 50,00 |
Total: | 100,00 |
designation | Time (hours) |
---|---|
Estudo autónomo | 72,00 |
Frequência das aulas | 30,00 |
Trabalho escrito | 60,00 |
Total: | 162,00 |
The final mark is the average of the results obtained in modules A and B (topics to be defined in due time). The evaluation in each topic will be defined by the lecturer. In the current year the evaluation is done in the following way:
There is no option to improve the final mark.