Slide 1The hard X-ray spectrum of Pulsar Wind Nebulae Data-models comparison in the Simbol-X era F. Bocchino, INAF Osservatorio Astronomico di Palermo with contributions…

Slide 11 Information and Surveillance Systems for Refugee Populations Gilbert Burnham, MD, PhD Johns Hopkins University Slide 2 2 Section A The Need for Information and Data…

Slide 1Max- Planck- Institut fuer extr. Physik and and Astrophysics Dept, University of Oxford Slide 2 Slide 3 light year light year x km/s light year x km parsec) parsec)…

Slide 1Dissipation in Force-Free Astrophysical Plasmas Hui Li (Los Alamos National Lab) Radio lobe formation and relaxation Dynamical magnetic dissipation in force-free plasmas:…

Slide 1Astro-2: History of the Universe Lecture 2; April 6 2006 Slide 2 Previously.. On Astro-2 The goal of cosmology is to understand how the universe formed and evolved.…

Slide 1accessing RAVE hardware for PLATO PIC Ulisse Munari Tomaz Zwitter Slide 2 RAVEspectroscopy 8400-8800 Å range 8400-8800 Å range 7500 resolving power 7500 resolving…

Slide 1Galaxy feedback in 3D Roberto Maiolino Slide 2 Feedback is the key: - reducing SF efficiency (gas heating+turbulence) - removing baryons Discrepancy between halo mass…

Slide 11)Are disks predicted? Theories of HM SF 2)Are disks observed? Search methods 3)Observational evidence disks VS toroids 4)Open questions and the future: ALMA, etc.…

Slide 1Astrometry of Water Masers in Post-AGB Stars Hiroshi Imai Graduate School of Science and Engineering, Kagoshima University Slide 2 Contents Astrometry with VLBA, and…

Slide 1The PRIMA facility: Phase-Referenced Imaging and Micro-arcsecond Astrometry Slide 2 Plan PRIMA Principle Scientific objectives Physical limitations –Off-axis angle…