T 90: Gammaastronomie 2
  Tuesday, February 28, 2012, 16:45–19:10, ZHG 008
  
    
  
  
    
      
        
          
            
              |  | 16:45 | T 90.1 | Group Report:
            
            
              
                (contribution withdrawn) Observations of the Crab pulsar with the MAGIC telescope — •Takayuki Saito, Gianluca Giavitto, Stefan Klepser, Thomas Schweizer, Eckart Lorenz, Razmick Mirzoyan, and Masahiro Teshima | 
        
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              |  | 17:05 | T 90.2 | Group Report:
            
            
              
                Observations of the Crab pulsar and the Crab Nebula with the MAGIC telescopes — •Takayuki Saito, Emiliano Carmona, Gianluca Giavitto, Stefan Klepser, Daniel Mazin, Thomas Schweizer, Julian Sitarek, and Roberta Zanin | 
        
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              |  | 17:25 | T 90.3 | (contribution withdrawn) Giant radio pulses of the Crab pulsar - A multiwavelength study with MAGIC and several radio facilities — Natalia Lewandowska, •Dominik Elsässer, and Karl Mannheim | 
        
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              |  | 17:40 | T 90.4 | Supernovaüberreste mit Fermi und H.E.S.S. — •Anneli Schulz, Michael Mayer, Markus Ackermann und Christian Stegmann | 
        
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              |  | 17:55 | T 90.5 | Very-high-energy gamma-radiation from supernova remnants as seen with H.E.S.S. — •Joachim Hahn, Anne Bochow, Henning Gast, Vincent Marandon, and Matthieu Renaud | 
        
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              |  | 18:10 | T 90.6 | Röntgenanalyse und Modellierung des Pulsarwindnebels G21.5-0.9 — •Philipp Willmann, Peter Eger, Felix Fürst, Markus Holler, Kathrin Valerius, Jörn Wilms, Ira Jung und Christian Stegmann | 
        
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              |  | 18:25 | T 90.7 | Modellierung der Breitbandemission von Pulsarwindnebeln — •Michael Mayer, Julia Brucker, Ira Jung, Kathrin Valerius und Christian Stegmann | 
        
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              |  | 18:40 | T 90.8 | New Chandra results of the complex unidentified TeV source HESSJ1841-055 — •Sven Wilbert, Omar Tibolla, and Sarah Kaufmann | 
        
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              |  | 18:55 | T 90.9 | Models for γ ray emission in W51 — Sara Rebecca Gozzini, •Fabian Jankowski, and Wlodek Bednarek | 
        
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