array(2) { ["lab"]=> string(3) "484" ["research"]=> string(3) "771" } Black hole accretion, jet formation, and wind - 黑洞吸积与高能天体物理研究组 | LabXing

黑洞吸积与高能天体物理研究组

黑洞吸积与高能天体物理研究组由袁峰研究员领导，目前有三名副研究员，三名博士后，八名学生和一名实习生。

中国科学院 / 上海天文台

Black hole accretion, jet formation, and wind

Black hole accretion is a fundamental physical process in the universe and is the primary power source behind active galactic nuclei (AGNs), black hole binaries (BHBs), and, possibly, gammaray bursts.Black hole accretion flows can be divided into two broad classes: cold and hot.Observations show that hot accretion flows are associated with jets. In addition, theoretical arguments suggest that hot flows should produce strong winds. 

                                                                                                                                                                  

创建: May 14, 2018 | 11:59