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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 1.

MB vs. ﹩{\rm{\Delta }}{M}_{15}(B)﹩ for our entire grid of 4500 models. The relationship of Phillips et al. (1999) is overplotted as a red box. Models with ﹩{\rm{\Delta }}{M}_{15}(B)\geqslant 1.55﹩ are definitively sub-﹩{M}_{\mathrm{ch}}﹩. Both ﹩{M}_{\mathrm{ch}}﹩, sub-﹩{M}_{\mathrm{ch}}﹩, and even some super-﹩{M}_{\mathrm{ch}}﹩ models are consistent with ﹩0.8\lt {\rm{\Delta }}{M}_{15}(B)\lt 1.55﹩.

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