On the Ca-strong 1991bg-like type Ia supernova 2016hnk: evidence for a Chandrasekhar-mass explosion
Creators: name: Galbany, Lluís
name: Ashall, Chris
name: Hoeflich, Peter
name: González-Gaitán, Santiago
name: Taubenberger, Stefan
name: Stritzinger, Maximilian
name: Hsiao, Eric Y.
name: Mazzali, Paolo
name: Baron, Eddie
name: Blondin, Stéphane
name: Bose, Subhash
name: Bulla, Mattia
name: Burke, Jamison F.
name: Burns, Christopher R.
name: Cartier, Régis
name: Chen, Ping
name: Della Valle, Massimo
name: Diamond, Tiara R.
name: Gutiérrez, Claudia P.
name: Harmanen, Jussi
name: Hiramatsu, Daichi
name: Holoien, T. W. -S.
name: Hosseinzadeh, Griffin
name: Howell, D. Andrew
name: Huang, Yiwen
name: Inserra, Cosimo
name: de Jaeger, Thomas
name: Jha, Saurabh W.
name: Kangas, Tuomas
name: Kromer, Markus
name: Lyman, Joseph D.
name: Maguire, Kate
name: Marion, George Howie
name: Milisavljevic, Dan
name: Prentice, Simon J.
name: Razza, Alessandro
name: Reynolds, Thomas M.
name: Sand, David J.
name: Shappee, Benjamin J.
name: Shekhar, Rohit
name: Smartt, Stephen J.
name: Stassun, Keivan G.
name: Sullivan, Mark
name: Valenti, Stefano
name: Villanueva, Steven
name: Wang, Xiaofeng
name: Wheeler, J. Craig
name: Zhai, Qian
name: Zhang, Jujia
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences
subject: FOS: Physical sciences

description: We present a comprehensive dataset of optical and near-infrared photometry and spectroscopy of type~Ia supernova (SN) 2016hnk, combined with integral field spectroscopy (IFS) of its host galaxy, MCG -01-06-070, and nearby environment. Properties of the SN local environment are characterized by means of single stellar population synthesis applied to IFS observations taken two years after the SN exploded. SN 2016hnk spectra are compared to other 1991bg-like SNe Ia, 2002es-like SNe Ia, and Ca-rich transients. In addition, abundance stratification modelling is used to identify the various spectral features in the early phase spectral sequence and the dataset is also compared to a modified non-LTE model previously produced for the sublumnious SN 1999by. SN 2016hnk is consistent with being a sub-luminous (M$_{\rm B}=-16.7$ mag, s$_{\rm BV}$=0.43$\pm$0.03), highly reddened object. IFS of its host galaxy reveals both a significant amount of dust at the SN location, as well as residual star formation and a high proportion of old stellar populations in the local environment compared to other locations in the galaxy, which favours an old progenitor for SN 2016hnk. Inspection of a nebular spectrum obtained one year after maximum contains two narrow emission lines attributed to the forbidden [Ca II] $λλ$7291,7324 doublet with a Doppler shift of 700 km s$^{-1}$. Based on various observational diagnostics, we argue that the progenitor of SN 2016hnk was likely a near Chandrasekhar-mass ($M_{\rm Ch}$) carbon-oxygen white dwarf that produced 0.108 $M_\odot$ of $^{56}$Ni. Our modeling suggests that the narrow [Ca II] features observed in the nebular spectrum are associated with $^{48}$Ca from electron capture during the explosion, which is expected to occur only in white dwarfs that explode near or at the $M_{\rm Ch}$ limit.
description: 23 pages, 27 figures. A&amp;A accepted