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  Evidence for a Chandrasekhar-mass explosion in the Ca-strong 1991bg-like type Ia supernova 2016hnk

Galbany, L., Ashall, C., Höflich, P., González-Gaitán, S., Taubenberger, S., Stritzinger, M., et al. (2019). Evidence for a Chandrasekhar-mass explosion in the Ca-strong 1991bg-like type Ia supernova 2016hnk. Astronomy and Astrophysics, 630: A76. doi:10.1051/0004-6361/201935537.

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Item Permalink: http://hdl.handle.net/21.11116/0000-0004-D6D2-D Version Permalink: http://hdl.handle.net/21.11116/0000-0004-D6D3-C
Genre: Journal Article


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Galbany, L., Author
Ashall, C., Author
Höflich, P., Author
González-Gaitán, S., Author
Taubenberger, S.1, Author              
Stritzinger, M., Author
Hsiao, E. Y., Author
Mazzali, P.1, Author              
Baron, E., Author
Blondin, S., Author
Bose, S., Author
Bulla, M., Author
Burke, J. F., Author
Burns, C. R., Author
Cartier, R., Author
Chen, P., Author
Valle, M. Della, Author
Diamond, T. R., Author
Gutiérrez, C. P., Author
Harmanen, J., Author
Hiramatsu, D., AuthorHoloien, T. W.-S., AuthorHosseinzadeh, G., AuthorHowell, D. Andrew, AuthorHuang, Y., AuthorInserra, C., Authorde Jaeger, T., AuthorJha, S. W., AuthorKangas, T., AuthorKromer, M., AuthorLyman, J. D., AuthorMaguire, K., AuthorMarion, G. Howie, AuthorMilisavljevic, D., AuthorPrentice, S. J., AuthorRazza, A., AuthorReynolds, T. M., AuthorSand, D. J., AuthorShappee, B. J., AuthorShekhar, R., AuthorSmartt, S. J., AuthorStassun, K. G., AuthorSullivan, M., AuthorValenti, S., AuthorVillanueva, S., AuthorWang, X., AuthorWheeler, J. Craig, AuthorZhai, Q., AuthorZhang, J., Author more..
1Stellar Astrophysics, MPI for Astrophysics, Max Planck Society, ou_159882              


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 Abstract: Aims. 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. Our goal with this complete dataset is to understand the nature of this peculiar object. Methods. 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. We performed detailed analyses of SN photometric data by studying its peculiar light and color curves. SN 2016hnk spectra were compared to other 1991bg-like SNe Ia, 2002es-like SNe Ia, and Ca-rich transients. In addition, we used abundance stratification modeling to identify the various spectral features in the early phase spectral sequence and also compared the dataset to a modified non-LTE model previously produced for the sublumnious SN 1999by. Results. SN 2016hnk is consistent with being a subluminous (MB = −16.7 mag, sBV=0.43 ± 0.03), highly reddened object. The IFS of its host galaxy reveals both a significant amount of dust at the SN location, residual star formation, and a high proportion of old stellar populations in the local environment compared to other locations in the galaxy, which favors 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] λλ7291,7324 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 (MCh) carbon-oxygen white dwarf that produced 0.108 M of 56Ni. Our modeling suggests that the narrow [Ca II] features observed in the nebular spectrum are associated with 48Ca from electron capture during the explosion, which is expected to occur only in white dwarfs that explode near or at the MCh limit.


 Dates: 2019-08-05
 Publication Status: Published online
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Method: -
 Identifiers: DOI: 10.1051/0004-6361/201935537
Other: LOCALID: 3169403
 Degree: -



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Title: Astronomy and Astrophysics
  Other : Astron. Astrophys.
Source Genre: Journal
Publ. Info: France : EDP Sciences S A
Pages: - Volume / Issue: 630 Sequence Number: A76 Start / End Page: - Identifier: ISSN: 1432-0746
CoNE: https://pure.mpg.de/cone/journals/resource/954922828219_1