Speaker
Radomir Smida
(Karlsruhe Institute of Technology)
Description
Arrival directions of ultra-high energy cosmic rays
from the direction to one of the brightest radio source Virgo A were studied with recent models of the Galactic magnetic field. The obtained image of this radiogalaxy is similar for all studied models and it is unique in the comparison with images of other
possible point source candidates. We present a method suitable for identifying cosmic rays arriving from this close-by radiogalaxy.
| Registration number following "ICRC2015-I/" | 0180 |
|---|---|
| Collaboration | -- not specified -- |
Primary author
Radomir Smida
(Karlsruhe Institute of Technology)
Co-authors
Daniel Bub
(Karlsruhe Institute of Technology)
Dr
Engel Ralph
(Karlsruhe Institute of Technology)
