Magnetars are highly magnetized neutron stars; their formation mechanism is unknown. Hot helium-rich stars with spectra dominated by emission lines are known as Wolf-Rayet stars. We observe the binary system HD 45166 using spectropolarimetry, finding that it contains a Wolf-Rayet star with a mass of 2 solar masses and a magnetic field of 43 kilogauss. Stellar evolution calculations indicate that this component will explode as a type Ib or IIb supernova, and the strong magnetic field favors a magnetar remnant. We propose that the magnatized Wolf-Rayet star formed by the merger of two lower mass helium stars.
@article{arxiv.2308.08591,
title = {A massive helium star with a sufficiently strong magnetic field to form a magnetar},
author = {T. Shenar and G. A. Wade and P. Marchant and S. Bagnulo and J. Bodensteiner and D. M. Bowman and A. Gilkis and N. Langer and A. -N. Chene and L. Oskinova and T. Van Reeth and H. Sana and N. St-Louis and A. Soares de Oliveira and H. Todt and S. Toonen},
journal= {arXiv preprint arXiv:2308.08591},
year = {2023}
}
Comments
Published in Science on the 18 August 2023. Radial velocities, spectra, and software available in: https://zenodo.org/record/8042656 ESO press release: www.eso.org/public/news/eso2313