arXiv Open Access 2025

PISN 2018ibb: radioactive emission of [O III] lines

Nikolai N. Chugai
Lihat Sumber

Abstrak

Supernova 2018ibb of the PISN category related to the dynamical instability of oxygen core in a supermassive star induced by pair-creation shows at the nebular stage strong [\oiii] emission lines of an uncertain origin. I propose a simple model that demonstrates a possibility of [O III] lines emission from the supernova oxygen matter ionized and heated by the $^{56}$Co radioactive decay. The reason is pinpointed by which the [O III] line luminosity among supernovae of PISN category can vary in a broad range.

Topik & Kata Kunci

Penulis (1)

N

Nikolai N. Chugai

Format Sitasi

Chugai, N.N. (2025). PISN 2018ibb: radioactive emission of [O III] lines. https://arxiv.org/abs/2501.07134

Akses Cepat

Lihat di Sumber
Informasi Jurnal
Tahun Terbit
2025
Bahasa
en
Sumber Database
arXiv
Akses
Open Access ✓