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A massive helium star with a sufficiently strong magnetic field to form a magnetar

Tijdschriftbijdrage - Tijdschriftartikel

Magnetars are highly magnetized neutron stars, the formation mechanism of which is unknown. Hot helium-rich stars with spectra dominated by emission lines are known as Wolf-Rayet stars. We observed the binary system HD 45166 using spectropolarimetry and reanalyzed its orbit using archival data. We found that the system 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 supernova, and that its magnetic field is strong enough for the supernova to leave a magnetar remnant. We propose that the magnetized Wolf-Rayet star formed by the merger of two lower-mass helium stars.
Tijdschrift: Science
ISSN: 0036-8075
Issue: 6659
Volume: 381
Pagina's: 761 - 765
Jaar van publicatie:2023
Toegankelijkheid:Open