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SN 2020uem: a Possible Thermonuclear Explosion within a Dense Circumstellar Medium. I. The Nature of Type IIn/Ia-CSM SNe from Photometry and Spectroscopy

  • Authors: Kohki Uno, Keiichi Maeda, Takashi Nagao, Tatsuya Nakaoka, Kentaro Motohara, Akito Tajitsu, Masahiro Konishi, Shuhei Koyama, Hidenori Takahashi, Masaomi Tanaka, Hanindyo Kuncarayakti, Miho Kawabata, Masayuki Yamanaka, Kentaro Aoki, Keisuke Isogai, Kenta Taguchi, Mao Ogawa, Koji S. Kawabata, Yuzuru Yoshii, Takashi Miyata, Ryo Imazawa

Kohki Uno et al 2023 The Astrophysical Journal 944 .

  • Provider: AAS Journals

Caption: Figure 15.

Time evolution of the carbon dust mass. We gathered data from Li et al. (2022), Maeda et al. (2013) (SN IIn: 2010jl), and Stritzinger et al. (2012) (SNe IIn: 2005ip and 2006jd). The symbols are different for different spectral types of SNe; IIn (circles), IIn/Ia-CSM (diamonds), 2005ip and 2006jd (squares), and 2020uem (star). The open symbols show the upper limits of dust mass, while the filled symbols show confirmed dust mass.

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