Image Details

Choose export citation format:

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 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.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse