Galactic X-ray binary jets

Elena Gallo

doi:10.1007/s10509-007-9571-z

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arXiv · 0705.0014

Galactic X-ray binary jets

Elena Gallo

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Abstract

With their relatively fast variability time-scales, Galactic X-ray binaries provide an excellent laboratory to explore the physics of accretion and related phenomena, most notably outflows, over different regimes. After comparing the phenomenology of jets in black hole X-ray binary systems to that of neutron stars, here I discuss the role of the jet at very low Eddington ratios, and present preliminary results obtained by fitting the broadband spectral energy distribution of a quiescent black hole binary with a `maximally jet-dominated' model.

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Elena Gallo. 2007-06-26. Galactic X-ray binary jets. https://doi.org/10.1007/s10509-007-9571-z

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