Evidence for Sub-Chandrasekhar Mass Type Ia Supernovae from an Extensive Survey of Radiative Transfer Models
Authors: Daniel A. Goldstein, and Daniel Kasen
2018 The Astrophysical Journal Letters852L33.
Provider: AAS Journals
Caption: Figure 3.
SEDONA light curves for the models that lie along the WLR (red boxed region in Figure 1), color-coded by ﹩{M}_{{}^{56}\mathrm{Ni}}﹩. There is a strong correlation between light-curve shape and ﹩{M}_{{}^{56}\mathrm{Ni}}﹩ in all bands.