Second Maximum of SN 2019stc: Collision with a Circumstellar Shell?

Variable thermal energy injection from magnetar spin-down as a possible cause of stripped-envelope supernova light-curve bumps

(2022) Takashi J Moriya et al.   MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

Bumpy Declining Light Curves Are Common in Hydrogen-poor Superluminous Supernovae

(2022) Griffin Hosseinzadeh et al.   ASTROPHYSICAL JOURNAL

Electron acceleration in supernova remnants

(2022) Artem Bohdan   PLASMA PHYSICS AND CONTROLLED FUSION

The Luminous and Double-peaked Type Ic Supernova 2019stc: Evidence for Multiple Energy Sources

(2021) Sebastian Gomez et al.   ASTROPHYSICAL JOURNAL

SN 2008iy circumstellar interaction: bright and lesser light effects

(2021) N N Chugai   MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

Origin of postmaximum bump in luminous type Ic SN 2019stc

(2021) Nikolai N Chugai et al.   Monthly Notices of the Royal Astronomical Society: Letters

The Most Luminous Supernovae

(2019) Avishay Gal-Yam   Annual Review of Astronomy and Astrophysics

SUPERNOVA LIGHT CURVES POWERED BY YOUNG MAGNETARS

(2010) Daniel Kasen et al.   ASTROPHYSICAL JOURNAL

BRIGHT SUPERNOVAE FROM MAGNETAR BIRTH

(2010) S. E. Woosley   Astrophysical Journal Letters