Astrophysical magnetohydrodynamical outflows in the extragalactic binary system LMC X-1

Abstract

In this work, at first we present a model of studying astrophysical flows of binary systems and microquasars based on the laws of relativistic magnetohydrodynamics. Then, by solving the time independent transfer equation, we estimate the primary and secondary particle distributions within the hadronic astrophysical jets as well as the emissivities of high energy neutrinos and $\gamma$-rays. One of our main goals is, by taking into consideration the various energy-losses of particles into the hadronic jets, to determine through the transport equation the respective particle distributions focusing on relativistic hadronic jets of binary systems. As a concrete example we examine the extragalactic binary system LMC X-1 located in the Large Magellanic Cloud, a satellite galaxy of our Milky Way Galaxy.

arXiv comment6 pages, 6 figures, submitted to Journal of Physics: Conference Series

References in corpus (6)

• Energy spectra of gamma-rays, electrons and neutrinos produced at proton-proton interactions in the very high energy regime
• The Mass of the Black Hole in Cygnus X-1
• A New Dynamical Model for the Black Hole Binary LMC X-1
• Magnetic field effects on neutrino production in microquasars
• Production of gamma rays and neutrinos in the dark jets of the microquasar SS433
• Dynamical and radiative simulations of $\gamma$-ray jets in microquasars

Cited by in corpus (2)

• Simulations of neutrino and gamma-ray production from relativistic black-hole microquasar jets
• Relativistic Magnetized Astrophysical Plasma Outflows in Black-Hole Microquasars