Constraining Type Iax supernova progenitor systems with stellar population age dating

Tyler Takaro*, Ryan J. Foley, Curtis McCully, Wen Fai Fong, Saurabh W. Jha, Gautham Narayan, Armin Rest, Maximilian Stritzinger, Kevin McKinnon

*Corresponding author for this work

Research output: Contribution to journalArticle

1 Scopus citations

Abstract

Type Iax supernovae (SNe Iax) are the most common class of peculiar SNe. While they are thought to be thermonuclear white-dwarf (WD) SNe, SNe Iax are observationally similar to, but distinct from SNe Ia. Unlike SNe Ia, where roughly 30 per cent occur in early-type galaxies, only one SN Iax has been discovered in an early-type galaxy, suggesting a relatively short delay time and a distinct progenitor system. Furthermore, one SN Iax progenitor system has been detected in pre-explosion images with its properties consistent with either of two models: a short-lived (<100 Myr) progenitor system consisting of a WD primary and a Hestar companion, or a singularWolf-Rayet progenitor star. Using deep Hubble Space Telescope images of nine nearby SN Iax host galaxies, we measure the properties of stars within 200 pc of the SN position. The ages of local stars, some of which formed with the SN progenitor system, can constrain the time between star formation and SN, known as the delay time. We compare the local stellar properties to synthetic photometry of single-stellar populations, fitting to a range of possible delay times for each SN.With this sample, we uniquely constrain the delay-time distribution for SNe Iax, with a median and 1σ confidence interval delay time of 63+58-15 × 106 yr. The measured delay-time distribution provides an excellent constraint on the progenitor system for the class, indicating a preference for a WD progenitor system over a Wolf-Rayet progenitor star.

Original languageEnglish (US)
Pages (from-to)986-1002
Number of pages17
JournalMonthly Notices of the Royal Astronomical Society
Volume493
Issue number1
DOIs
StatePublished - Mar 1 2020

Keywords

  • Supernovae: general
  • Supernovae: individual (SN 2008A, SN 2008ge, SN 2008ha, SN 2010ae, SN 2010el, SN 2011ay, SN 2012Z, SN 2014ck, SN 2014dt)

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Fingerprint Dive into the research topics of 'Constraining Type Iax supernova progenitor systems with stellar population age dating'. Together they form a unique fingerprint.

  • Cite this

    Takaro, T., Foley, R. J., McCully, C., Fong, W. F., Jha, S. W., Narayan, G., Rest, A., Stritzinger, M., & McKinnon, K. (2020). Constraining Type Iax supernova progenitor systems with stellar population age dating. Monthly Notices of the Royal Astronomical Society, 493(1), 986-1002. https://doi.org/10.1093/mnras/staa294