The Progenitor and Early Evolution of the Type IIb SN 2016gkg
2017
We report initial observations and analysis on the Type IIb SN 2016gkg
in the nearby galaxy NGC 613. SN 2016gkg exhibited a clear double-peaked
light curve during its early evolution, as evidenced by our intensive
photometric follow-up campaign. SN 2016gkg shows strong similarities
with other Type IIb SNe, in particular, with respect to the He i
emission features observed in both the optical and near-infrared. SN
2016gkg evolved faster than the prototypical Type IIb SN 1993J, with a
decline similar to that of SN 2011dh after the first peak. The analysis
of archival Hubble Space Telescope images indicate a pre-explosion
source at SN 2016gkg’s position, suggesting a progenitor star with
a ˜mid-F spectral type and initial mass 15{--}20 M {}⊙
, depending on the distance modulus adopted for NGC 613. Modeling
the temperature evolution within 5 {days} of explosion, we obtain a
progenitor radius of ˜ 48{--}124 R {}⊙ , smaller
than that obtained from the analysis of the pre-explosion images
(240{--}320 R {}⊙ ).
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