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SN 2017dio: A Type-Ic Supernova Exploding in a Hydrogen-rich Circumstellar Medium

  • Authors: Hanindyo Kuncarayakti, Keiichi Maeda, Christopher J. Ashall, Simon J. Prentice, Seppo Mattila, Erkki Kankare, Claes Fransson, Peter Lundqvist, Andrea Pastorello, Giorgos Leloudas, Joseph P. Anderson, Stefano Benetti, Melina C. Bersten, Enrico Cappellaro, Régis Cartier, Larry Denneau, Massimo Della Valle, Nancy Elias-Rosa, Gastón Folatelli, Morgan Fraser, Lluís Galbany, Christa Gall, Avishay Gal-Yam, Claudia P. Gutiérrez, Aleksandra Hamanowicz, Ari Heinze, Cosimo Inserra, Tuomas Kangas, Paolo Mazzali, Andrea Melandri, Giuliano Pignata, Armin Rest, Thomas Reynolds, Rupak Roy, Stephen J. Smartt, Ken W. Smith, Jesper Sollerman, Auni Somero, Brian Stalder, Maximilian Stritzinger, Francesco Taddia, Lina Tomasella, John Tonry, Henry Weiland, and David R. Young

2018 The Astrophysical Journal Letters 854 L14.

  • Provider: AAS Journals

Caption: Figure 3.

(Left) Comparison of the CSM interaction-subtracted spectrum of SN 2017dio (red) with spectra of other SNe (black; including SNID templates of Modjaz et al. 2014). (Right) Comparison of the +6 day spectrum of SN 2017dio (red) with those of other SNe combined with interaction spectrum (black; fV = 0.3), a template SN Ic+CSM interaction spectrum from Leloudas et al. (2015, green), and SN 2012ca (orange). The spectrum of SN 1994I combined with the interaction spectrum (fV = 0.1) is showed for comparison with SN 2017dio at +18 days. The comparison spectra are from WISeREP. In both panels, phases are days from maximum for spectra other than SN 2017dio.

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