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19 April 2024
 
  » arxiv » 1502.0646

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Constraining the Progenitor Companion of the Nearby Type Ia SN 2011fe with a Kiloday Nebular Spectrum
Melissa L. Graham ; Peter E. Nugent ; Mark Sullivan ; Alexei V. Filippenko ; S. Bradley Cenko ; Jeffrey M. Silverman ; Kelsey I. Clubb ; Weikang Zheng ;
Date 26 Jan 2015
AbstractWe present a "kiloday" optical nebular spectrum of the nearby Type Ia supernova (SN) 2011fe, obtained +981 days after explosion. SN 2011fe exhibits little evolution since the +593 day optical spectrum, but there are several curious aspects in this new extremely late-time regime. We see new emission features at 5800 and 6400 AA that could be attributed to [Fe I], but also consider (and reject) the possibility that the latter is the high-velocity hydrogen predicted by Mazzali et al. (2014). The nebular feature at 5200 AA exhibits a linear velocity evolution of $sim350$ $ m km s^{-1}$ per 100 days from at least +220 to +980 days, but the line’s shape also changes in this time, suggesting that line blending contributes to the evolution. At $sim 1000$ days after explosion, flux from the SN has declined to a point where contribution from a hot, luminous secondary could be detected. In this work we make the first observational tests for a post-impact remnant star and constrain its luminosity to $<(3-5) imes 10^3$ $ m L_{odot}$. Additionally, we do not see any evidence for narrow H$alpha$ emission, placing an upper limit of $3 imes 10^{-4}$ $ m M_{odot}$ on the mass of hydrogen in the system. We conclude that observations continue to strongly exclude many single-degenerate scenarios for SN 2011fe.
Source arXiv, 1502.0646
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