Speaker
袁峰
(Shanghai Astronomical Observatory)
Description
The hard and quiescent states of black hole X-ray binaries and most supermassive black holes in the nearby universe are powered by hot accretion flows. In this talk, I will review wind and jet launched from this type of accretion flow, including both their theoretical studies and observaitonal evidences. For winds, we will introduce their launching mechanism and main properties such as mass flux and velocity. For jets, in addition to the continuous jets, we will focus more on the formation mechanism of epsodic jets and the associated flares.
| Topic | X射线双星 |
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Primary author
袁峰
(Shanghai Astronomical Observatory)
