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 4.
Correlation between ﹩{M}_{{}^{56}\mathrm{Ni}}﹩ and peak brightness for models off the WLR (blue squares) and on the WLR (orange dots). The quadratic fitting functions in Equations (8)–(11) are plotted as black dashed lines in each panel.