Speaker
Guillaume DUBUS
(IPAG CNRS/Université Grenoble Alpes)
Description
The presence of a relativistic pulsar wind has been established in several X-ray binaries. The interaction of the pulsar wind with the stellar companion, stellar wind, or accretion disk can lead to peculiar signatures, most prominently the emission of high-energy gamma-rays. I will describe our efforts to model this interaction in order to translate gamma-ray observations into a better understanding of relativistic magnetized outflows.
Author
Guillaume DUBUS
(IPAG CNRS/Université Grenoble Alpes)
