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.
A., et al., 2020, @doi [Monthly Notices of the Royal Astronomical Society] 10.1093/mnras/staa2241 , 498, 25
1 Pith paper cite this work, alongside 26 external citations. Polarity classification is still indexing.
1
Pith paper citing it
26
external citations · OpenAlex
fields
astro-ph.IM 1years
2025 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
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.