Galactic X-ray binary jets |
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Authors: | Elena Gallo |
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Institution: | (1) University of California, Santa Barbara, CA 93106, USA |
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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 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.
Chandra Fellow |
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Keywords: | X-rays: binaries Radiation mechanisms: general Stars: individual (A0620– 00) |
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