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The Physics of the Nebular Phase in Black Hole X-ray Binaries: Modelling V404 Cygni
Some of the most extreme galactic black hole transients exhibit a nebular phase at the end of their outbursts. This stage was first identified in the 2015 outburst of V404 Cygni, when it dominated the optical spectrum for ~4 days. It is characterised by exceptionally strong optical emission lines, t
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