PPT-Numerical Studies of Accretion Disks, Jets, and Gamma Ray B

Author : stefany-barnette | Published Date : 2016-02-26

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

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Numerical Studies of Accretion Disks, Jets, and Gamma Ray B: Transcript

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 highenergy Xray radio and visible radiation that are observable from great distances across the universe. Alecian Abstract In this chapter I 64257rst present the premain sequence stars around which accretion disks are observed and summarise the main observed characteristics of the classical T Tauri and Herbig AeBe stars I then review the theoretical and Formation and cosmic evolution of massive black holes. Andrea Merloni. MPE, Garching. Syllabus. Monday:. Observational evidence of Supermassive Black Holes. AGN surveys. Tuesday: . The evolution of SMBH mass function and spin distributions. 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. 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. The View From Telescopes, Computers. and the Lab. Adam Frank. University of Rochester. A Cast Of Lots and Lots. AstroBEAR development. : J. Carroll, B. . Lui. , M. . Huarte. -Espinosa, S. Li, E. Hanson, E. Kaminski, K. . 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. Optical polarization monitoring of OJ 287 in 2005 - 2009. . Carolin. . Villforth. (Turku & . STScI. ), Kari . Nilsson . (Turku), . Jochen. . Heidt. (LSW Heidelberg) . + 45 . . 6. /27/12. In collaboration with . Avi. Loeb. Harvard University Astronomy Department. arXiv:. 1109.6660, PRL 108, 6, 061302. Observing . Lense-Thirring. Precession in Tidal Disruption Flares. Outline. Phil Armitage. Colorado. Motivation. What can we directly observe?. Dust. m. m-mm. Gas – . emission &. kinematics. (CO other. molecules, . H. 2. hard). Limited. direct . time . dependence. Evolution. 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). M87. Studying the Cosmos through..... . Observations. Theory. Experiment. Astro @ Purdue. Astro @ Purdue. 9 . research-active faculty members covering a wide range of topics. Group includes postdoctoral scholars, staff scientists and students. Theory. Mario Livio. Space Telescope Science Institute. Which Systems Have Highly Collimated . Jets. ?. Object . Physical System. Young Stellar Objects. Accreting Star. HMXBs. Accreting NS or BH. X-ray Transients.

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