Rotation in shrapnel from a supernova

An artist’s impression of the explosion and subsequent ejection of a partly burnt runaway star like LP 40-365 (credit University of Warwick/Mark Garlick).

In June 2021 work led by researchers in the BU White Dwarf group discovered that the partly burnt runaway star LP 40-365 (also known as GD 492) rotates every 8.9 hours using archival data from the Transiting Exoplanet Survey Satellite (TESS) and the Hubble Space Telescope (HST) published as Hermes, Putterman, Hollands, et al. 2021. This relatively long rotation period likes adds more evidence that LP 40-365 is actually the bound remnant of an exploded white dwarf itself, the still-simmering embers of a thermonuclear (Type Iax) explosion that slung-shot the star from the Milky Way. An excellent write-up was recently featured in The Brink, and a thread on the discovery of the system is located here: https://twitter.com/jotajotahermes/status/1394298751087435784?s=20. The paper has been published the Astrophysical Journal Letters.

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