HK 39: Nuclear Astrophysics III
  Tuesday, March 17, 1998, 17:00–19:00, E
  
    
  
  
    
      
        
          
            
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          17:00 | 
          HK 39.1 | 
          
            
            
              
                Anisotropic angular distribution of the 6Li(d,α)4He reaction below 60 keV — •D. Bemmerer, A. Biller, K. Czerski, P. Heide, M. Hoeft, A. Huke, and G. Ruprecht
              
            
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          17:15 | 
          HK 39.2 | 
          
            
            
              
                The 15N(p,α)12C reaction in the stellar energy range from 65 to 345 keV — •C. Herrmann, K. Czerski, P. Heide, M. Hoeft, and C. Reineke
              
            
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          17:30 | 
          HK 39.3 | 
          
            
              Group Report:
            
            
              
                Investigation of the reactions 19F(p,αγ)16O and 19F(p,γ)20Ne relevant for the recycling/breakout of the CNO cycles 1.0mm♣ — •J.W. Hammer, R. Ott, G. Bulski, M. Jaeger, A. Mayer, R. Kunz, R. Morlock, G. Staudt, K. Spyrou, Ch. Chronidou, S. Harissopulos, T. Paradellis, H. Schulte, and C. Rolfs
              
            
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          18:00 | 
          HK 39.4 | 
          
            
            
              
                Discovery of the astrophysically interesting 3/2+ state of 19F at Ex = 7101 keV — •J.W. Hammer, Y. Butt, P. Parker, M. Jaeger, R. Kunz, A. Mayer, R. Schreiter, and G. Staudt
              
            
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          18:15 | 
          HK 39.5 | 
          
            
            
              
                Helium Burning of 22Ne: The Reaction 22Ne(α,γ)26Mg — •M. Jaeger, J. W. Hammer, A. Mayer, R. Kunz, R. Morlock, V. Koelle, and G. Staudt
              
            
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          18:30 | 
          HK 39.6 | 
          
            
            
              
                Neutron Capture of 26Mg: Direct Capture and Resonances * — •P. Mohr, H. Beer, and H. Oberhummer
              
            
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          18:45 | 
          HK 39.7 | 
          
            
            
              
                Der stellare Neutroneneinfangquerschnitt von 34S — •René Reifarth, Franz Käppeler und Kilian Schwarz
              
            
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