Modeling the X-ray Contribution of X-ray Binary Jets

Details Modeling the X-ray Contribution of X-ray Binary Jets Modeling the X-ray Contribution of X-ray Binary Jets

2003-01-23

arxiv.org/abs/astro-ph/0301479v1

New Astron.Rev. 47 (2003) 491-493

Astronomy and Astrophysics

Astrophysics

4 pages, 1 Table, conference proceedings for "The Physics of Relativistic Jets in the Chandra and XMM Era, Bologna, 2002", Eds

Scientific paper

10.1016/S1387-6473(03)00078-2

Astrophysical jets exist in both XRBs and AGN, and seem to share common features, particularly in the radio. While AGN jets are known to emit X-rays, the situation for XRB jets is not so clear. Radio jets have been resolved in several XRBs in the low/hard state, establishing that some form of outflow is routinely present in this state. Interestingly, the flat-to-inverted radio synchrotron emission associated with these outflows strongly correlates with the X-ray emission in several sources, suggesting that the jet plasma plays a role at higher frequencies. In this same state, there is increasing evidence for a turnover in the IR/optical where the flat-to-inverted spectrum seems to connect to an optically thin component extending into the X-rays. We discuss how jet synchrotron emission is likely to contribute to the X-rays, in addition to inverse Compton up-scattering, providing a natural explanation for these correlations and the turnover in the IR/optical band. We present model parameters for fits to several sources, and address some common misconceptions about the jet model.

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