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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 Letters 852 L33.

  • 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.

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