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Explosive Nucleosynthesis in Aspherical Hypernova Explosions and Late Time Spectra of SN1998bw

K. Maeda·T. Nakamura·K. Nomoto·P. A. Mazzali·F. Patat·I. Hachisu
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Abstract

Aspherical explosion models for the hypernova (hyper-energetic supernova) SN 1998bw are presented. Nucleosynthesis in aspherical explosions is examined with a two-dimensional hydrodynamical code and a detailed nuclear reaction network. Aspherical explosions lead to a strong $α$-rich freezeout, thus enhancing the abundance ratios [$^{44}$Ca, $^{48}$Ti, and $^{64}$Zn / Fe] in the ejecta. The nebular line profiles of the Fe-dominated blend near 5200 Åand of [\OI] 6300,6363 Åare calculated and compared with the observed late time spectra of SN 1998bw. Compared with the spherical model, the unusual features of the observed nebular spectra can be better explained if SN 1998bw is a strongly aspherical explosion with a kinetic energy of $\sim 10^{52}$ ergs viewed from near the jet direction.

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K. Maeda, T. Nakamura, K. Nomoto, P. A. Mazzali, F. Patat, I. Hachisu. 2001-09-27. Explosive Nucleosynthesis in Aspherical Hypernova Explosions and Late Time Spectra of SN1998bw. https://arxiv.org/abs/astro-ph/0011003

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