Luminous red novae show electron-scattering wings and Case B recombination deviations, indicating shock interaction with dense circumstellar material powers these transients.
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Luminous Red Novae as shock-powered transients I: Electron-scattering wings and deviations from Case B
Luminous red novae show electron-scattering wings and Case B recombination deviations, indicating shock interaction with dense circumstellar material powers these transients.