An eclipsing 47 min double white dwarf binary at 400 pc
Abstract
We present the discovery of the eclipsing double white dwarf (WD) binary WDJ 022558.21-692025.38 that has an orbital period of 47.19 min. Following identification with the Transiting Exoplanet Survey Satellite, we obtained time series ground based spectroscopy and high-speed multiband ULTRACAM photometry which indicate a primary DA WD of mass and a mass secondary WD, which is likely of type DA as well. The system becomes the third-closest eclipsing double WD binary discovered with a distance of approximately 400 pc and will be a detectable source for upcoming gravitational wave detectors in the mHz frequency range. Its orbital decay will be measurable photometrically within 10 yr to a precision of better than 1 per cent. The fate of the binary is to merge in approximately 41 Myr, likely forming a single, more massive WD.
Department(s)
Physics, Astronomy, and Materials Science
Document Type
Article
DOI
10.1093/mnras/stad2347
Keywords
binaries: close, gravitational waves, stars: individual: WDJ 022558.21-692025.38, white dwarfs
Publication Date
10-1-2023
Recommended Citation
Baran, Andrzej S.; Munday, James; Tremblay; Hermes; Barlow, Brad; Pelisoli, Ingrid; Marsh; Parsons, Steven G.; Jones, David; Kepler; Brown, Alex; Littlefair; Hegedus; Breedt, Elme;; and Dhillon, "An eclipsing 47 min double white dwarf binary at 400 pc" (2023). Faculty Scholarship. 542.
https://bearworks.missouristate.edu/articles00/542
Journal Title
Monthly Notices of the Royal Astronomical Society