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What can we learn from Neutron Star X-Ray Binaries' JETS?
Authors:Simone Migliari  Rob Fender
Institution:(1) University of Amsterdam, Amsterdam, The Netherlands;(2) University of Southampton, Southampton, United Kingdom
Abstract:We review our current knowledge of the disk-jet coupling in neutron star X-ray binaries. We compare neutron star and black hole X-ray binaries, by means of radio and X-ray observations, in order to understand the role played in the production of the jet, by characteristics proper of the accreting compact object involved: the existence of a solid surface, the presence of an ergosphere/event horizon, the strength of the magnetic field, the spin of the compact object.
Keywords:binaries  close  stars  jets and outflows  radio continuum
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