PPT-A warm mode of accretion

Author : candy | Published Date : 2023-10-27

in simulations of galaxy formation G Murante INAF OATo P Monaco Univ Ts M Calabrese SISSA Ts G De Lucia INAF OATs S Borgani Univ Ts K

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A warm mode of accretion: Transcript

in simulations of galaxy formation G Murante INAF OATo P Monaco Univ Ts M Calabrese SISSA Ts G De Lucia INAF OATs S Borgani Univ Ts K . 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. X-ray binaries. Rudy . Wijnands. Anton . Pannekoek. Institute for Astronomy. University of Amsterdam. 3 August 2015. Lorentz center, Leiden. Low- versus high-mass X-ray binaries. Low-mass X-ray binaries. 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. between . XRB. and . AGN. . Accretion . Processes. Anca. . Constantin. James Madison Univ.. W/. Paul . Green(SAO. ) . Tom . Aldcroft. (SAO. ). HongYan. . Zhou(USTChina. ). Daryl Haggard (. UWashington. 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. . ). Planetesimals and Protoplanets. Planetesimals. There are three processes that take place which bring solid bits of matter – rocks, metal, and ice – into larger bodies called . planetesimals.. Planetesimals. 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-. Nathalie . Degenaar. . University of Michigan. X-ray observations. Interior properties. Thermal evolution. Quiescence. No/little accretion. Neutron star visible. Accretion outburst. Rapid accretion. Paul A. Mason. New Mexico State University. Emmanuel Gonzalez. University of Texas at El Paso. Edward L. Robinson. University of Texas at . Austin. Special thanks to . Jorge I. Zuluaga . for discussion on time-scale estimates. . and Outburst Mechanisms. Zhaohuan. Zhu. Hubble Fellow, Princeton University. Collaborators: Lee Hartmann (. Umich. ), Charles . Gammie. (UIUC), . . Nuria. . Calvet. (. Umich. Priyamvada Natarajan . Yale University. . Volonteri. ; Johnson. ; Park ; . Ricotti. ; . Khochfar. ; Di . Matteo. ; Yoshida ; . Haiman. ; Tanaka ; . Schneider Dubois ; . Bournoud. ; Loeb ; . 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). 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. XRB. and . AGN. . Accretion . Processes. Anca. . Constantin. James Madison Univ.. W/. Paul . Green(SAO. ) . Tom . Aldcroft. (SAO. ). HongYan. . Zhou(USTChina. ). Daryl Haggard (. UWashington. ).

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