Optical rms spectra of the black hole transient V404 Cygni show wind-related P-Cygni profiles as inverted shapes, providing a new variability-based wind diagnostic.
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Accretion disc winds imprint distinct signatures in the optical variability spectrum of black hole transients
Optical rms spectra of the black hole transient V404 Cygni show wind-related P-Cygni profiles as inverted shapes, providing a new variability-based wind diagnostic.