PPT-The nature of the accretion flow in AGN

Author : ximena | Published Date : 2024-02-09

Prof Chris Done University of Durham amp ISASJAXA AGN feedback MagorrianGebhardt relation gives BH mass Big black holes live in host galaxies with big bulges Either

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The nature of the accretion flow in AGN: Transcript

Prof Chris Done University of Durham amp ISASJAXA AGN feedback MagorrianGebhardt 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 . 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. 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. between . XRB. and . AGN. . Accretion . Processes. Anca. . Constantin. James Madison Univ.. W/. Paul . Green(SAO. ) . Tom . Aldcroft. (SAO. ). HongYan. . Zhou(USTChina. ). Daryl Haggard (. UWashington. Neutron Star Binaries and Its Implications. QCS2014@2014.10.20. Chang-Hwan Lee @. 1. Nuclear Physics A 928 (2014) 296. (. 李昌桓. ). Prakash (2013). All well measured NS masses in NS-NS binaries are < 1.5 . effects on ices:. studies with a chemo-dynamical model. Jeong-Eun Lee. Kyung . Hee. University. University of Texas at Austin. Contents:. Very Low Luminosity Objects (. VeLLOs. , L<0.1. L. . ). 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-. My main PhD simulations were performed on COSMOS Mk I in 1998-99!. 32 R10000, 8 GB of memory, $2,000,000. 0.5×10. 6. particles, only 4,000 . timesteps. Simulations I’ll talk about today, 32 core servers, with 64 GB, $20,000. Chapter 8:. Outflow and Accretion. Yosuke Mizuno. Institute of Astronomy. National . Tsing-Hua. University. Outflow and Accretion. In the universe, . outflow. and . accretion. are common feature.. Kazuya Takahashi. with Yu Yamamoto, . Shoichi. Yamada. (. Waseda. Univ.). Outline. Introduction. My research. Results. Standing Accretion Shock Instability (SASI). New points. How?. Non-spherical structures in progenitors. and Outburst Mechanisms. Zhaohuan. Zhu. Hubble Fellow, Princeton University. Collaborators: Lee Hartmann (. Umich. ), Charles . Gammie. (UIUC), . . Nuria. . Calvet. (. Umich. Flow in Aquifers – 2 Unconfined Aquifer Flow Groundwater Hydraulics Daene C. McKinney 1 Summary Unconfined Aquifer Flow Continuity Equation Steady Horizontal Flow Steady Horizontal Flow with Infiltration Aggregate Analysis In A CubeSat Centrifuge: A Study Of Primary Accretion Sarah Smallwood Faculty Mentor: Erik Asphaug , School of Earth and Space Exploration Graduate Student Mentor: Elizabeth Dyer XRB. and . AGN. . Accretion . Processes. Anca. . Constantin. James Madison Univ.. W/. Paul . Green(SAO. ) . Tom . Aldcroft. (SAO. ). HongYan. . Zhou(USTChina. ). Daryl Haggard (. UWashington. ). studies with a chemo-dynamical model. Jeong-Eun Lee. Kyung . Hee. University. University of Texas at Austin. Contents:. Very Low Luminosity Objects (. VeLLOs. , L<0.1. L. . ). Episodic accretion & Chemistry (Lee 2007).

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