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Physics of Relativistic Flows
Physics of Relativistic Flows
from 04 May 2009 to 13 June 2009 Nordita
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(no code) Supercritical phenomena in relativistic flows
(no code) Physics of Relativistic Flows: An observational view
(no code) Physics of Relativistic Flows: An observational view
(no code) Physics of Relativistic Flows: An observational view
--not specified--
   Contribution List (47) showing 1-20
 
Id Date Type upTitle Presenter Session Track
286 2009-May-27 12:45   discussion   no code  
296 2009-Jun-10 11:00   Convective instability of relativistic, decelerating ejecta : an origin of magnetic fields in the early afterglow phase? LEVINSON, Amir    
279 2009-May-20 13:15   Constraints on the parameters of efficiently radiating relativistic jets Dr. DERISHEV, Evgeny    
291 2009-May-26 10:30   Conditions for launching of relativistic jets in GRBs BARKOV, Maxim    
273 2009-May-18 10:30   coffee discussion      
264 2009-May-12 10:30   coffee discussion      
252 2009-May-05 10:30   coffee discussion      
266 2009-May-13 10:30   coffee discussion      
251 2009-May-04 15:15   coffee discussion      
250 2009-May-04 10:30   coffee discussion      
262 2009-May-08 15:15   coffee discussion      
263 2009-May-11 10:30   coffee discussion      
276 2009-May-20 10:30   coffee discussion      
270 2009-May-15 15:15   coffee discussion      
255 2009-May-06 10:30   coffee discussion      
289 2009-Jun-12 10:30   Black-Hole Jets of Ultrahigh Energy Cosmic Rays: Clues from Auger and Fermi DERMER, Charles    
290 2009-May-27 12:30   Automatic quenching of high energy gamma--ray sources by synchrotron photons STAWARZ, Lukasz no code  
285 2009-May-27 12:00   Astrophysical implications of photon breeding mechanism POUTANEN, Juri no code  
257 2009-May-07 13:15   A Role and a Structure of the Magnetic Field in Jets, Hotspots and Lobes of Radio Galaxies Dr. STAWARZ, Lukasz    
272 2009-May-19 10:30   A model of the TeV flare of Cygnus X-1: electron acceleration and extended pair cascades Dr. ZDZIARSKI, Andrzej    
showing 1-20
 

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