PPT-The Magnetic Origin of Black Hole Accretion Disk Winds

Author : yoshiko-marsland | Published Date : 2019-11-28

The Magnetic Origin of Black Hole Accretion Disk Winds Chris Shrader NASA Goddard Space Flight Center Collaborators D Kazanas GSFC K Fukumura JMU F Tombesi UMD

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The Magnetic Origin of Black Hole Accretion Disk Winds: Transcript

The Magnetic Origin of Black Hole Accretion Disk Winds Chris Shrader NASA Goddard Space Flight Center Collaborators D Kazanas GSFC K Fukumura JMU F Tombesi UMD Ehud Behar . Thermodynamics with Lambda: Some Consequences. L. David . Kubiz. ňák. (Perimeter Institute). . Lambda and Quasi-Lambda workshop. University of Massachusetts, Amherst, MA, USA. April 10 – April 12, 2014. Ramesh Narayan. Jets are Widespread. Relativistic Jets . occur widely in . accreting black holes (BHs): AGN, XRBs, GRBs. A . common . robust . mechanism . must be producing all these . Jets. Best Bet. Christopher C. Lindner, . Milos. . Milosavljevic. , Sean Couch, . Pawan. Kumar. . The University of Texas at Austin. Results. We have conducted hydrodynamic simulations of the viscous post-core-collapse accretion of a rapidly rotating 14 solar mass Wolf-. Optical polarization monitoring of OJ 287 in 2005 - 2009. . Carolin. . Villforth. (Turku & . STScI. ), Kari . Nilsson . (Turku), . Jochen. . Heidt. (LSW Heidelberg) . + 45 . i. What causes wind? . Caused by a difference in air pressure due to. unequal heating of the atmosphere.. Winds are created by. ….. • . Heating the air, decreases pressure (warm. air rises creating a low pressure). Yi-Hsieh Wang, Ted Jacobson, Mark Edwards, and Charles W. Clark. arXiv:1705.01907 . Black hole explosions?. Experimental black-hole evaporation?. Black hole lasers. Implementation in Bose-Einstein condensates. and Outburst Mechanisms. Zhaohuan. Zhu. Hubble Fellow, Princeton University. Collaborators: Lee Hartmann (. Umich. ), Charles . Gammie. (UIUC), . . Nuria. . Calvet. (. Umich. Ted Jacobson. University of Maryland. Gravity and Black Holes, Cambridge, July 4, 2017 . Wheeler to . Bekenstein. (1971):. “If I drop a teacup into a black hole, . I conceal from all the world the. Pawel. . Artymowicz. U of Toronto. MRI turbulence. Some non-MRI turbulence. Roles and the dangers of turbulence. UCSC Santa Cruz 2010. I borrowed some . figures & slides from. X. Wu (2004). R. Nelson (2008). L. David . Kubiz. ňák. (Perimeter Institute). . Lambda and Quasi-Lambda workshop. University of Massachusetts, Amherst, MA, USA. April 10 – April 12, 2014. Plan of the talk. Black holes as thermodynamic objects . Screw And Surface. Counterbore. Countersink. Threaded hole. Clearance Hole. Zhaohuan. Zhu. Hubble Fellow, Princeton University. Collaborators: Lee Hartmann (. Umich. ), Charles . Gammie. (UIUC), . . Nuria. . Calvet. (. Umich. ), Jonathan McKinney (UMD),. . and the . Blazar. Sequence. . Demos . Kazanas, Chris Shrader (NASA/GSFC). Keigo Fukumura, Sean Scully (JMU). Markos Georganopoulos (UMBC). (based on work by Fukumura, Kazanas, Contopoulos, Behar. Prof Chris Done. University . of Durham & ISAS/JAXA. AGN feedback. Magorrian-Gebhardt. relation gives BH mass!! Big black holes live in host galaxies with big bulges! Either measured by bulge luminosity or bulge mass (stellar velocity dispersion) or .

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