Microquasars are X-ray binaries with relativistic jets. These jets are powerful energy carriers—
thought to be fed by accretion—which produce nonthermal emission at different energy …

Bayesian inference provides a simple and unified approach to data analysis, allowing
experimenters to assign probabilities to competing hypotheses of interest, on the basis of the …

Abstract Very high energy\(\gamma\)-rays are one of the most important messengers of the
relativistic non-thermal Universe. The major motivation of very high energy\(\gamma\)-ray …

We present a new edition of the catalogue of high-mass X-ray binaries in the Galaxy. The
catalogue contains source name (s), coordinates, finding chart, X-ray luminosity, system …

Microquasars are binary star systems with relativistic radio-emitting jets. They are potential
sources of cosmic rays and can be used to elucidate the physics of relativistic jets. We report …

We systematically investigate the effects of high supernova kick velocities on the orbital
parameters of post-supernova neutron-star binaries. Using Monte Carlo simulations, we …

X-ray binaries are composed of a normal star in orbit around a neutron star or stellar-mass
black hole. Radio and x-ray observations have led to the presumption that some x-ray …

Context. LS 5039 and LS I+ 61° 303 are unique amongst high-mass X-ray binaries (HMXB)
for their spatially-resolved radio emission and their counterpart at> GeV gamma-ray …

Black hole gravitohydromagnetics (GHM) is developed from the rudiments to the frontiers of
research in this book. GHM describes plasma interactions that combine the effects of gravity …

The binary star LS I+ 61 303 is remarkable for its periodic radio outbursts every 26.5 days.
We recently discovered a∼ 4.4 yr periodic modulation of the phase and amplitude of these …