 | Study programme 2018-2019 | Français | |
 | Astrophysique stellaire | ||
Programme component of Master's Degree in Physics à la Faculty of Science |
| Code | Type | Head of UE | Department’s contact details | Teacher(s) |
|---|---|---|---|---|
| US-M1-SCPHYS-012-M | Optional UE | N. | SSERV - Aucun service |
|
| Language of instruction | Language of assessment | HT(*) | HTPE(*) | HTPS(*) | HR(*) | HD(*) | Credits | Weighting | Term |
|---|---|---|---|---|---|---|---|---|---|
| Français | 30 | 0 | 0 | 0 | 0 | 4 | 4.00 | 1st term |
| AA Code | Teaching Activity (AA) | HT(*) | HTPE(*) | HTPS(*) | HR(*) | HD(*) | Term | Weighting |
|---|---|---|---|---|---|---|---|---|
| S-PHYS-205 | Stellar Astrophysics | 30 | 0 | 0 | 0 | 0 | Q1 | 100.00% |
| Programme component |
|---|
Objectives of Programme's Learning Outcomes
Type of Teaching Activity/Activities
| AA | Type of Teaching Activity/Activities |
|---|---|
| S-PHYS-205 |
|
Mode of delivery
| AA | Mode of delivery |
|---|---|
| S-PHYS-205 |
|
Required Reading
| AA | |
|---|---|
| S-PHYS-205 |
Required Learning Resources/Tools
| AA | Required Learning Resources/Tools |
|---|---|
| S-PHYS-205 | Not applicable |
Recommended Reading
| AA | |
|---|---|
| S-PHYS-205 |
Recommended Learning Resources/Tools
| AA | Recommended Learning Resources/Tools |
|---|---|
| S-PHYS-205 | - S.L. Shapiro and S.A Teukolsky, Black Holes, White Dwarfs and Neutron Stars, The Physics of Compact Objects; - C.E. Rolfs and W.S. Rodney, Cauldrons in the Cosmos - CI. D.D. Clayton, Principles of Stellar Evolution and Nucleosynthesis, - C.J. Hansen, S.D. Kawaler and V. Trimble, Stellar Interiors |
Other Recommended Reading
| AA | Other Recommended Reading |
|---|---|
| S-PHYS-205 | Not applicable |
Grade Deferrals of AAs from one year to the next
| AA | Grade Deferrals of AAs from one year to the next |
|---|---|
| S-PHYS-205 | Unauthorized |
(*) HT : Hours of theory - HTPE : Hours of in-class exercices - HTPS : hours of practical work - HD : HMiscellaneous time - HR : Hours of remedial classes. - Per. (Period), Y=Year, Q1=1st term et Q2=2nd term