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What can we Learn from the Rising Light Curves of Radioactively Powered Supernovae?

  • Authors: Anthony L. Piro and Ehud Nakar

Piro & Nakar 2013 The Astrophysical Journal 769 67.

  • Provider: AAS Journals

Caption: Figure 5.

Inferred mass, mass fraction, and depth of 56Ni in PTF 10vgv for different explosion times. The 56Ni mass M 56 is inferred from Equation (6), and we only plot M 56 and X 56 for times at which the bolometric luminosity cannot be explained as a diffusive tail according to Figure 4. The mass fraction is estimated as X 56M 56M diff, where the diffusion depth is calculated according to Equation (8).

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