TY  - GEN
UR  - https://archiv.ub.uni-heidelberg.de/volltextserver/11625/
Y1  - 2010///
ID  - heidok11625
KW  - H.E.S.S.-Experiment 
KW  -  TriggerSupernova Remnant 
KW  -  Cosmic Ray 
KW  -  Gamma-ray Astronomy 
KW  -  Imaging Atmospheric Cerenkov Telescope
N2  - Supernova remnants (SNRs) are the remainders of extremely energetic explosions occurring at the end of a star's life. With the energy released during the supernova explosion they are believed to accelerate charged particles to energies of up to 10^15 eV. In the very-high-energy (VHE, > 10^11 eV) gamma-ray band, SNRs represent one of the most populous classes of Galactic sources. Due to its unprecedented sensitivity, H.E.S.S. was the first instrument to allow for a morphological resolution of individual SNRs, proving the existence of particle acceleration and subsequent VHE gamma-ray emission. However, to date many more SNRs are known in the radio waveband than in VHE gamma-rays. This work presents a systematic study of the VHE gamma-ray signal of a sample of around 200 radio SNRs. The VHE gamma-ray-signal of these SNRs is studied individually. Besides the spatial correlation of radio SNRs and VHE gamma-ray sources, the measured flux of VHE gamma-rays is compared to theoretical flux predictions. These predictions are based on assumptions of the total explosion energy, the particle acceleration effciency, the density of the surrounding medium and the distance of the SNRs. The results presented here suggest that these parameters can vary strongly for individual SNRs. Future observations of SNRs in VHE gamma-rays and other wavebands will help to constrain the parameter space and will allow to further discuss acceleration mechanisms in SNRs.
AV  - public
A1  - Bochow, Anne
TI  - A systematic study of Supernova Remnants as seen with H.E.S.S.
ER  -