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Supernova Explosions of Super-asymptotic Giant Branch Stars: Multicolor Light Curves of Electron-capture Supernovae

  • Authors: Nozomu Tominaga, Sergei I. Blinnikov, and Ken'ichi Nomoto

Tominaga, Blinnikov, & Nomoto 2013 The Astrophysical Journal Letters 771 L12.

  • Provider: AAS Journals

Caption: Figure 4.

(a) Bolometric light curves of the ECSNe. The colors are the same as Figure  1, but the red line shows the energy release rate of the 56Co radioactive decay. (b) Multicolor light curves (red: u, green: g, blue: r, magenta: i, cyan: z, yellow: J, black: H, and gray: K) of the ECSN of the SAGB star with M env = 3.0  M and X env(H) = 0.2. (c) Bolometric light curves of the ECSNe without the pulsar contribution (red), with the full deposition (green), and with the one-group transport (blue). The energy release rate of the 56Co radioactive decay (gray) is also shown.

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