PPT-10/28/2010 SEAL@GSFC 1 MHD Accretion-Disk Winds

and the Blazar Sequence Demos Kazanas Chris Shrader NASAGSFC Keigo Fukumura Sean Scully JMU Markos Georganopoulos UMBC based on work by Fukumura Kazanas Contopoulos Behar. Universal Accretion Laboratories. Rob Hynes (LSU). Christian Knigge. University of Southampton. Outline. Cataclysmic variables. A. primer. CVs as universal accretion disk laboratories. From phenomenology to physics. Phil Armitage. Colorado. Processes in Protoplanetary Disks. Disk structure. Disk evolution. Turbulence. Episodic accretion. Single particle evolution. Ice lines and persistent radial structure. Transient structures in disks. Gamma ray bursts (GRB) are an especially exciting outflow phenomena that are capable of outputting as much energy as our sun will. Christopher C. . Lindner. 1. Abstract. Relativistic Jets are streams of plasma moving throughout the universe at speeds up to 99% the speed of light. They produce high-energy X-ray, radio, and visible radiation that are observable from great distances across the universe. young stars . with . LSST. Gregory J. Herczeg. KIAA. Star Formation: . ISM/Molecular Clouds . Pre-main sequence stellar evolution. (low-mass case). HD141569, . Clampin. et al.. Classical T . Tauri. Stars. 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-. Phil Armitage. Colorado. Processes in Protoplanetary Disks. Disk structure. Disk evolution. Turbulence. Episodic accretion. Single particle evolution. Ice lines and persistent radial structure. Transient structures in disks. 1. MHD Accretion-Disk Winds as . AGN X-ray Absorbers. . ~ . Seyfert. galaxies to quasars ~. Demos Kazanas Keigo Fukumura . Astrophysics . Science . Division Code . 663, . NASA/GSFC. Ehud Behar (. 1. MHD Accretion-Disk Winds . . 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. and Outburst Mechanisms. Zhaohuan. Zhu. Hubble Fellow, Princeton University. Collaborators: Lee Hartmann (. Umich. ), Charles . Gammie. (UIUC), . . Nuria. . Calvet. (. Umich. 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 ( 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 ( The . Mid-Infrared Evolution of the FU Orionis . Disk. Green . et al. 2016, . ApJ. , 832, . 4. Instrument: FORCAST. Background. FU Ori is the canonical example of an FU Orionis object, a class of stars that undergo sudden brightening events . Centaurus. A. July 15, 2010: Accretion Workshop. Cambridge, Massachusetts. Gregory R. Sivakoff (. UVa. ). Chandra . Cen. . A-. Very Large Project Team. A Galaxy’s Cookbook. A Population of X-Ray Binaries. Zhaohuan. Zhu. Hubble Fellow, Princeton University. Collaborators: Lee Hartmann (. Umich. ), Charles . Gammie. (UIUC), . . Nuria. . Calvet. (. Umich. ), Jonathan McKinney (UMD),.