Speaker
Mr
Stanislav Stefanik
(Institute of Particle and Nuclear Physics, Charles University)
Description
We examine temporal evolution of the observed $\gamma$-ray intensity from the direction of the
binary PSR B1259-63 using only numbers of detected very high energetic photons.
Simple and straightforward method is applied to the published data obtained with the
Imaging Atmospheric Cherenkov Technique during campaigns around three periastron passages of
the binary system.
Changes attributable to the variations of the intrinsic source activity were recognized at
high levels of significance.
Primary authors
Dr
Dalibor Nosek
(Institute of Particle and Nuclear Physics, Charles University)
Mr
Stanislav Stefanik
(Institute of Particle and Nuclear Physics, Charles University)
