Seven Years of SN 2014C: A Multiwavelength Synthesis of an Extraordinary Supernova
Abstract
SN 2014C was originally classified as a Type Ib supernova, but at phase ϕ = 127 days, post-explosion strong Hα emission was observed. SN 2014C has since been observed in radio, infrared, optical and X-ray bands. Here we present new optical spectroscopic and photometric data spanning ϕ = 947-2494 days post-explosion. We address the evolution of the broadened Hα emission line, as well as broad [O III] emission and other lines. We also conduct a parallel analysis of all publicly available multiwavelength data. From our spectra, we find a nearly constant Hα FWHM velocity width of ~2000 km s-1 that is significantly lower than that of other broadened atomic transitions (~3000-7000 km s-1) present in our spectra ([O I] λ6300; [O III] λ λ4959, 5007; He I λ7065; [Ca II] λ λ7291, 7324). The late radio data demand a fast forward shock (~10,000 km s-1 at ϕ = 1700 days) in rarified matter that contrasts with the modest velocity of the Hα. We propose that the infrared flux originates from a toroidal-like structure of hydrogen surrounding the progenitor system, while later emission at other wavelengths (radio, X-ray) likely originates predominantly from the reverse shock in the ejecta and the forward shock in the quasi-spherical progenitor He-wind. We propose that the Hα emission arises in the boundary layer between the ejecta and torus. We also consider the possible roles of a pulsar and a binary companion.
- Publication:
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The Astrophysical Journal
- Pub Date:
- May 2022
- DOI:
- 10.3847/1538-4357/ac5fa6
- arXiv:
- arXiv:2203.12747
- Bibcode:
- 2022ApJ...930...57T
- Keywords:
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- Supernovae;
- Type Ib supernovae;
- Type II supernovae;
- Circumstellar matter;
- Circumstellar disks;
- Circumstellar shells;
- X-ray transient sources;
- Radio transient sources;
- 1668;
- 1729;
- 1731;
- 241;
- 235;
- 242;
- 1852;
- 2008;
- Astrophysics - High Energy Astrophysical Phenomena
- E-Print:
- 33 pages, 12 figures