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

Author : basidell | Published Date : 2020-06-16

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

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

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. between . XRB. and . AGN. . Accretion . Processes. Anca. . Constantin. James Madison Univ.. W/. Paul . Green(SAO. ) . Tom . Aldcroft. (SAO. ). HongYan. . Zhou(USTChina. ). Daryl Haggard (. UWashington. 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., . 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. 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. 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 ; . 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 ( 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 ( Availableonlineatwww.sciencedirect.comScienceDirectFuzzySetsandSystems www.elsevier.com/locate/fss OWAWOWAfamiliesVicençTorraScience,MIT-building,University,Institute,University,IrelandSchoolUniversi XRB. and . AGN. . Accretion . Processes. Anca. . Constantin. James Madison Univ.. W/. Paul . Green(SAO. ) . Tom . Aldcroft. (SAO. ). HongYan. . Zhou(USTChina. ). Daryl Haggard (. UWashington. ). kindly visit us at www.nexancourse.com. Prepare your certification exams with real time Certification Questions & Answers verified by experienced professionals! We make your certification journey easier as we provide you learning materials to help you to pass your exams from the first try. Zhaohuan. Zhu. Hubble Fellow, Princeton University. Collaborators: Lee Hartmann (. Umich. ), Charles . Gammie. (UIUC), . . Nuria. . Calvet. (. Umich. ), Jonathan McKinney (UMD),. S.Dyussembekova. , . S.E.Kichanov. . , . J.Wasicki. , . W.Nawrocik. , . D.P.Kozlenko. ,. . N.M. . Belozerova. , B.N. . Savenko. 1. Figure 1. The ball-and-stick schematic representation of the molecule of ranitidine hydrochloride. . 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 .

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