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The top documents tagged [kpc slide]
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kpc slide
The 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.
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1 Information and Surveillance Systems for Refugee Populations Gilbert Burnham, MD, PhD Johns Hopkins University.
227 views
Max- Planck- Institut fuer extr. Physik and and Astrophysics Dept, University of Oxford.
219 views
Dissipation in Force-Free Astrophysical Plasmas Hui Li (Los Alamos National Lab) Radio lobe formation and relaxation Dynamical magnetic dissipation in.
213 views
Astro-2: History of the Universe Lecture 2; April 6 2006.
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Accessing RAVE hardware for PLATO PIC Ulisse Munari Tomaz Zwitter.
234 views
Galaxy feedback in 3D Roberto Maiolino. Feedback is the key: - reducing SF efficiency (gas heating+turbulence) - removing baryons Discrepancy between.
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1)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:
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Astrometry of Water Masers in Post-AGB Stars Hiroshi Imai Graduate School of Science and Engineering, Kagoshima University.
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The PRIMA facility: Phase-Referenced Imaging and Micro-arcsecond Astrometry.
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Cooling and Feedback in Early-Type Galaxies (and Groups) C. Jones, W. Forman, E. Churazov, P. Nulsen, R. Kraft X-ray emission from early-type galaxies.
213 views
X-ray Astronomy Group Richard Owen, Bob Warwick University of Leicester The X-ray Morphology and Spectra of Galactic Disks X-rays from Nearby Galaxies.
217 views
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