Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7399
Title: Flash Ionization Signatures in the Type Ibn Supernova SN 2019uo
Authors: Gangopadhyay, A
Misra, K
Hiramatsu, D
Wang, Shan-Qin
Hosseinzadeh, G
Wang, Xiaofeng
Valenti, Stefano
Zhang, Jujia
Howel, D. A
Arcavi, Iair
Anupama, G. C
Burke, Jamison
Dastidar, Raya
Koichi Itagaki, Koichi
Kumar, Brajesh
Kumar, B
Li, Long
McCully, Curtis
Mo, Jun
Pandey, S. B
Pellegrino, Craig
Sa, Hanna
Sahu, D. K
Pankaj Sanwal
Singh, A
Singh, M
Zhang, Jicheng
Zhang, Tianmeng
Zhang, Xinhan
Keywords: Core-collapse supernovae
Supernovae
CCD photometry
Photometry
Spectroscopy
Astronomical techniques
Issue Date: 1-Feb-2020
Publisher: IOP Publishing
Citation: The Astrophysical Journal, Vol. 889, No. 2, 170
Abstract: We present photometric and spectroscopic observations of the type Ibn supernova (SN) 2019uo, the second ever SN Ibn with flash ionization (He ii, C iii, N iii) features in its early spectra. SN 2019uo displays a rapid post-peak luminosity decline of 0.1 mag day−1 similar to most of the SNe Ibn, but is fainter(M max = - 18.30 + 0.24 mag) than a typical SN Ibn and shows a color evolution that places it between SNe Ib and the most extreme SNe Ibn. SN 2019uo shows P-cygni He i features in the early spectra which gradually evolve and become emission dominated post peak. It also shows faster evolution in line velocities as compared to most other members of the type Ibn subclass. The bolometric light curve is fairly well described by a 56Ni + circumstellar interaction model.
Description: Restricted Access
URI: http://prints.iiap.res.in/handle/2248/7399
ISSN: 0004-637X
Appears in Collections:IIAP Publications

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