Stellar mass loss (thermical velocities, mass loss rates), wind mechanisms, wind equation, pressure driven winds (sun, Parker solutions), radiation driven winds: a) hot stars, role of spectral lines, b) cool stars, dust driven stellar winds, numerical modelling, circumstellar envelopes of late-type stars, masers.
Sofern es die Pandemielage zulässt, soll diese Lehrveranstaltung als Präsenzveranstaltung durchgeführt werden. Informationen zum ONLINE Angebot sind ggf. unter https://www-astro.physik.tu-berlin.de zu finden.
Eligible lecture of the module „Advanced Astronomy and Astrophysics“ (Physics / Master). Open for all students with interest in astronomys and astrophysics.
Basic knowledge in Physics and Mathematics. Knowledge of the physics / B.Sc. Module „Einführung in die Astronomie und Astrophysik“ advised.
| Course No | Course Type | Hours |
|---|---|---|
| 20110501 | Vorlesung | 2 |
| Time Span | 19.10.2021 - 15.02.2022 |
|---|---|
| Instructors |
| 0352c_MA120 | 2020, MSc Physik (Mono), 120 LP |
| Day | Time | Location | Details |
|---|---|---|---|
| Tuesday | 12-14 | Online - zeitABhängig | 2021-10-19 - 2022-02-15 |