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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 7.

A high-dispersion spectrum of top of the narrow Hα profile, plotted in velocity space and with an arbitrary flux scale. We also show the rest wavelength in the top axis. The upper black spectrum shows a non-continuum-subtracted spectrum, while the lower black spectrum is a continuum-subtracted spectrum. The blue solid line shows an underlying broad component fit by a single Gaussian function. The solid orange line shows the double Gaussian components fit to the narrow P-Cygni component. The magenta vertical dashed line shows the rest wavelength of Hα (6562.8 Å). The cyan vertical dashed line shows a blueshift of −100 km s−1 from the rest wavelength, which corresponds to the absorption minimum of the P-Cygni profile. The apparent absorption at v ≈ −160 km s−1, which is shaded in gray, is an artifact, caused by bad pixels.

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