Viscous evolution models show circumbinary discs from binary mass transfer reach 0.07-0.20 solar masses and can explain dense CSM around fast-evolving Type Ibc SNe and FBOTs.
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Circumbinary Discs as the Origin of Circumstellar Material around Interacting H-poor Supernovae and Fast Blue Optical Transients
Viscous evolution models show circumbinary discs from binary mass transfer reach 0.07-0.20 solar masses and can explain dense CSM around fast-evolving Type Ibc SNe and FBOTs.