Radiation-hydrodynamic simulations of thermally-driven disc winds in X-ray binaries: A direct comparison to GRO J1655-40

Radiation-hydrodynamic simulations of thermally-driven disc winds in X-ray binaries: A direct comparison to GRO J1655-40

Essentially all low-mass X-ray binaries (LMXBs) in the soft state appear to drive powerful equatorial disc winds. A simple mechanism for driving such outflows involves X-ray heating of the top of the disc atmosphere to the Compton temperature. Beyond the Compton radius, the thermal speed exceeds the...

Bibliografske podrobnosti
Main Authors:	Higginbottom, N, Knigge, C, Long, KS, Matthews, JH, Sim, SA, Hewitt, HA
Format:	Journal article
Izdano:	Oxford University Press 2018

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