Wind-formed CV H-alpha profiles can populate the expected outflow region of the excess-EW diagram, but the diagram is so sensitive to wing definition that an FWHM-based mask and a calibrated EW scaling relation are proposed.
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A Diagnostic Kit for Optical Emission Lines Shaped by Accretion Disc Winds
Wind-formed CV H-alpha profiles can populate the expected outflow region of the excess-EW diagram, but the diagram is so sensitive to wing definition that an FWHM-based mask and a calibrated EW scaling relation are proposed.