A general introduction to the physics of binary star evolution. We start by the basic theory of determining binary star orbits and stellar masses. We investigate in detail mass transfer and mass loss from binary systems. An introduction to stellar evolution in binaries is given, before we focus on formation and evolution of high- and low-mass X-ray binaries and compare their observational properties with theory. We analyse radio pulsar binaries and binary systems with two compact objects (black holes, neutron stars, white dwarfs). We study kinematic effects of supernovae in binaries. Finally, we discuss gravitational waves and their astrophysical sources at low and high frequencies.
Lectures and exercises.
150 hours
Name of exam | High-Energy Astrophysics |
Type of exam | Written or oral exam |
ECTS | 5 |
Permitted aids | Information about allowed helping aids for the examination will be published in the description of the semester/module. |
Assessment | Passed/Not Passed |
Type of grading | Internal examination |
Criteria of assessment | The criteria of assessment are stated in the Examination Policies and Procedures |
Danish title | Højenergi astrofysik |
Module code | M-FYS-K3-3 |
Module type | Course |
Duration | 1 semester |
Semester | Autumn
|
ECTS | 5 |
Language of instruction | English |
Empty-place Scheme | Yes |
Location of the lecture | Campus Aalborg |
Responsible for the module |
Education owner | Master of Science (MSc) in Physics |
Study Board | Study Board of Mechanical Engineering and Physics |
Department | Department of Materials and Production |
Faculty | The Faculty of Engineering and Science |