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A Theory for the Maximum Magnitude versus Rate of Decline Relation of Classical Novae

  • Authors: Izumi Hachisu, Hideyuki Saio, Mariko Kato, Martin Henze, and Allen W. Shafter

2020 The Astrophysical Journal 902 91.

  • Provider: AAS Journals

Caption: Figure 8.

Same as Figure 5 but for the chemical composition of CO3. Each scaling mass (magenta lines) corresponds to the WD mass (from right to left, 0.55–﹩1.2\,{M}_{\odot }﹩ by ﹩0.05\,{M}_{\odot }﹩ steps, except ﹩0.98\,{M}_{\odot }﹩), the same as those tabulated in Table 1 (CO3). The thick magenta lines of equi-Msc (or equi-MWD) correspond to the WD mass region for CO novae (﹩{M}_{\mathrm{WD}}\leqslant 1.05\,{M}_{\odot }﹩).

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