Kavli Affiliate: Erin Kara | First 5 Authors: , , , , | Summary: Accretion discs in strong gravity ubiquitously produce winds, seen as blueshifted absorption lines in the X-ray band of both stellar mass X-ray binaries (black holes and neutron stars), and supermassive black holes. Some of the most powerful winds (termed Eddington winds) […]
Continue.. Stratified wind from a super-Eddington X-ray binary is slower than expected