PPT-The cold component of cluster accretion

Yuval Birnboim Jerusalem 2011 Clusters should be simple Abell 1689 Composite XrayChandra Optical HST The cooling flow Problem in Cool Core Clusters No cool lt1keV gas Star formation in brightest central galaxy lower by 10100 than expected from cooling. 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. 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 . 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-. component estimators in . the longitudinal data with multiple . sources . of . variation. . . & . Statistical Consulting Unit, ANU. ANU.  . Outline. Notation and Estimators. Bootstrap Methods. University of Sydney, . AAO, CAASTRO. SAMI instrument scientist. Hector project scientist. SAMI Galaxy Survey: . Gas/stellar misalignment . in . galaxies . and the . impact . of . morphology and environment. so much progress in the Chandra era. Alastair Edge. (Durham University). a. nd many collaborators. Cold?. This conference is primarily focused (rightly) on the X-ray regime so I should just define the parameters for this talk!. and Outburst Mechanisms. Zhaohuan. Zhu. Hubble Fellow, Princeton University. Collaborators: Lee Hartmann (. Umich. ), Charles . Gammie. (UIUC), . . Nuria. . Calvet. (. Umich. Creation of the United Nations. Organized in April 1945, the United Nations was intended to be a successor to the ineffective League of Nations.. The signatories of the charter dedicated themselves to maintaining peace and resolving potential conflicts without war.. Clustering, Dimensionality Reduction and Instance Based Learning Geoff Hulten Supervised vs Unsupervised Supervised Training samples contain labels Goal: learn All algorithms we’ve explored: Logistic regression Clustering, Dimensionality Reduction and Instance Based Learning Geoff Hulten Supervised vs Unsupervised Supervised Training samples contain labels Goal: learn All algorithms we’ve explored: Logistic regression so much progress in the Chandra era. Alastair Edge. (Durham University). a. nd many collaborators. Cold?. This conference is primarily focused (rightly) on the X-ray regime so I should just define the parameters for this talk!. Rudy . Wijnands. Anton . Pannekoek. Institute for Astronomy. University of Amsterdam. 15 December 2015. Texas Symposium 2015, Geneva. X-. ray. . luminosity. Quiescence. Outburst. Low-mass X-ray binary transients. 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. . HEDM of composite material . | . The cold-sprayed composite sample was illuminated with high energy x-rays, and the powder diffraction from the small grains of both constituent phases was recorded using large 2D detectors. The different phases have unique signatures in the x-ray diffraction owing to their different crystal structures, so the individual strain response of each phase can be independently observed. Macroscopic strain is monitored using digital image correlation cameras while the sample is under applied tensile load..