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. What is Whole Disk Encr yp tion Whole Disk Encr yp tion versus File Encr yp tion 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. College of Engineering. The University of Georgia. Development of an Embedded System for Assessing Extremity Blood Volumes based on Electrocardiography. Faculty Mentor: Zion Tsz Ho Tse. Graduate Mentor: T. Stan Gregory. 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. 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 (. Jets. (A Review with a Suggested Paradigm. ). David L. Meier. California Institute of Technology. The Innermost Regions of Relativistic Jets And Their Magnetic Fields. Granada, Spain; 10 June 2013. 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 ( 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. The soft tissue area . at. or . beyond. the junction of the hard and soft palates on which pressure, within . physiologic limits. , can be applied by a complete denture to aid in its retention.. Anatomic considerations. Category 5? typical gusts over open flat land of more than 280km/h. These winds correspond to the highest category on the Beaufort Scale. Extremely dangerous with widespread destruction. One of the