Page 1 IAP – Atelier Pulsar P. Laurent 16 Janvier 2006 1 SIMBOL-X Simbol-X Un observatoire dastrophysique X dur à lhorizon 2013 0.1–10 keV 15 keV-10 MeV 0.5 - 80 keV…

1. Silicon Drift Detectors for Synchrotron Energy Dispersive X-Ray Fluorescence Spectroscopy (SDD for EDXRF) Presentation by Dr. Saleh Qutaishat Petra University Amman –…

1. Silicon Drift Detectors for Synchrotron Energy Dispersive X-Ray Fluorescence Spectroscopy (SDD for EDXRF) Presentation by Dr. Saleh Qutaishat Petra University Amman –…

Slide 1 Experiments in X-Ray Physics Lulu Liu Partner: Pablo Solis Junior Lab 8.13 Lab 1 October 22nd, 2007 Slide 2 Discovery of X-Rays Wilhelm Roentgen (1895) image from…

Slide 1 NEI Modeling What do we have? What do we need? 2012.08.09 AtomDB workshop Hiroya Yamaguchi (CfA) Fe ion population in CIE (AtomDB v.2.0.2) Temperature (keV) Fe 24+…

Slide 1 The Galactic Center is a Treasure Box of High Energy Physics The Nearest AGN and Star Burst Galaxy. I will report a current picture of the Galactic Center, then move…

Snímek 1 On some prospects of the LOFT mission Institute of Physics, Silesian University in Opava Astronomical Institute, Prague Gabriel Török, Pavel Bakala, Vladimír…

Snímek 1 On Some Prospects of the LOFT Mission: QPO Models Institute of Physics, Silesian University in Opava Gabriel Török CZ.1.07/2.3.00/20.0071 Synergy , GAČR 209/12/P740,…

The cooling-flow problem Bremsstrahlung emission ) L / n2 ) center parts cool faster. Pressure equilibrium ) mass in-flow ) density increases. Mariano Mendez - SRON The cooling-flow…

The diffuse X-ray emission from the Galactic center      R. Belmont CESR, Toulouse, France Collaborators: M. Tagger (CEA/APC, France); M. Morris (UCLA, US); M. Muno…