Home Publications Research Grants Inventions & Patents Awards Additional Research Activities Faculties & Institutions Research Areas

Discovery of a Double-detonation Thermonuclear Supernova Progenitor

Kupfer T, Bauer EB, Van Roestel J, Bellm EC, Bildsten L, Fuller J, Prince TA, Heber U, Geier S, Green MJ, Kulkarni SR, Bloemen S, Laher RR, Rusholme B, Schneider D (2022)

---

Publication Type: Journal article

Publication year: 2022

Journal

Book Volume: 925

Journal Issue: 2

DOI: 10.3847/2041-8213/ac48f1

Abstract

We present the discovery of a new double-detonation progenitor system consisting of a hot subdwarf B (sdB) binary with a white dwarf companion with a P (orb) = 76.34179(2) minutes orbital period. Spectroscopic observations are consistent with an sdB star during helium core burning residing on the extreme horizontal branch. Chimera light curves are dominated by ellipsoidal deformation of the sdB star and a weak eclipse of the companion white dwarf. Combining spectroscopic and light curve fits, we find a low-mass sdB star, M (sdB) = 0.383 +/- 0.028 M (circle dot) with a massive white dwarf companion, M (WD) = 0.725 +/- 0.026 M (circle dot). From the eclipses we find a blackbody temperature for the white dwarf of 26,800 K resulting in a cooling age of approximate to 25 Myr whereas our MESA model predicts an sdB age of approximate to 170 Myr. We conclude that the sdB formed first through stable mass transfer followed by a common envelope which led to the formation of the white dwarf companion approximate to 25 Myr ago. Using the MESA stellar evolutionary code we find that the sdB star will start mass transfer in approximate to 6 Myr and in approximate to 60 Myr the white dwarf will reach a total mass of 0.92 M (circle dot) with a thick helium layer of 0.17 M (circle dot). This will lead to a detonation that will likely destroy the white dwarf in a peculiar thermonuclear supernova. PTF1 J2238+7430 is only the second confirmed candidate for a double-detonation thermonuclear supernova. Using both systems we estimate that at least approximate to 1% of white dwarf thermonuclear supernovae originate from sdB+WD binaries with thick helium layers, consistent with the small number of observed peculiar thermonuclear explosions.

Authors with CRIS profile

Involved external institutions

How to cite

APA:

Kupfer, T., Bauer, E.B., Van Roestel, J., Bellm, E.C., Bildsten, L., Fuller, J.,... Schneider, D. (2022). Discovery of a Double-detonation Thermonuclear Supernova Progenitor. Astrophysical Journal Letters, 925(2). https://dx.doi.org/10.3847/2041-8213/ac48f1

MLA:

Kupfer, Thomas, et al. "Discovery of a Double-detonation Thermonuclear Supernova Progenitor." Astrophysical Journal Letters 925.2 (2022).

BibTeX: Download