PPT-The high mass accretion rate spectra of GX 339-4:

Black hole spin from reflection Mari Kolehmainen amp Chris Done Durham University Maria Diaz Trigo ESO The Xray Universe 2011 Berlin Germany 27 30 June 2011 Black hole spin Specific angular momentum. 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. 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 . Conclusions. Barausse. E., 2012, MNRAS, 423, 2533. De . Rosa G., . Decarli. R., Walter . F.,Fan. X., Jiang L., Kirk J., . Pasquali A., . Rix. H. . W. ., 2011, . ApJ. , 739, 56;. F. an . X., Strauss M.A., Schneider D.P., Becker R.H., White R.L., . Phosphoproteomics. with Higher Energy . Collisional. Dissociation Fragmentation. Sangtae Kim. Ph.D. candidate. University of California, San Diego. C. enter for. C. omputational. M. ass. S. pectrometry. 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-. Sergey L. Sheetlin. ,. Yuri A. Mirokhin, Dmitrii V. Tchekhovskoi, Xiaoyu Yang, Stephen E. Stein. NIST Mass Spectrometry Data Center, Biomolecular Measurement Division,. National Institute of Standards and Technology. L~Ledd. accretion – BHB, ULX –. Chris Done, . ISAS/JAXA and University of Durham. Interacting . Binaries. - BRIGHT. High mass XRB & low mass XRB. Wind accretion – Messy. High mass companion star. and Outburst Mechanisms. Zhaohuan. Zhu. Hubble Fellow, Princeton University. Collaborators: Lee Hartmann (. Umich. ), Charles . Gammie. (UIUC), . . Nuria. . Calvet. (. Umich. Chris Done, . . University of Durham. Martin Ward, . Chichuan. Jin, Andreas Schultz. Kouchi. . Hagino. , . Aya. Kubota. Black holes are the simplest possible objects. Mass, spin. See them through accretion – . Sergey L. Sheetlin. ,. Yuri A. Mirokhin, Dmitrii V. Tchekhovskoi, Xiaoyu Yang, Stephen E. Stein. NIST Mass Spectrometry Data Center, Biomolecular Measurement Division,. National Institute of Standards and Technology. Zhaohuan. Zhu. Hubble Fellow, Princeton University. Collaborators: Lee Hartmann (. Umich. ), Charles . Gammie. (UIUC), . . Nuria. . Calvet. (. Umich. ), Jonathan McKinney (UMD),. Prof Chris Done. University . of Durham & ISAS/JAXA. AGN feedback. Magorrian-Gebhardt. 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 .