Image Details
Caption: Figure A1.
Comparison of our model bolometric lightcurves with those of existing models. The solid lines show our model results, while the dashed and dotted lines correspond to the models of A. L. Piro et al. (2021) and B. Margalit (2022), respectively. The green lines represent the case with rout = 1014 cm, χ = 1/7, MCSM = 10−1 M⊙, and vsh = 0.033c, while the orange and blue lines correspond to rout = 3.2 × 1014 and 1013 cm, respectively, with all other parameters unchanged. For consistency, we note that we adopt an opacity of κ = 0.34 cm2 g−1 in this comparison.
© 2026. The Author(s). Published by the American Astronomical Society.