Type Ibn supernovae arise from low-energy explosions of compact stars with ~1 solar mass ejecta and ~0.1 solar mass helium-rich circumstellar material, favoring binary progenitors over single massive stars.
(2012), [9] Hosseinzadeh et al
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Characterization of type Ibn SNe
Type Ibn supernovae arise from low-energy explosions of compact stars with ~1 solar mass ejecta and ~0.1 solar mass helium-rich circumstellar material, favoring binary progenitors over single massive stars.