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

• 成果类型: Article
• 署名作者: Shenar, Tomer; Wade, Gregg A.; Marchant, Pablo; Bagnulo, Stefano; Bodensteiner, Julia; Bowman, Dominic M.; Gilkis, Avishai; Langer, Norbert; Nicolas-Chene, Andre; Oskinova, Lidia; Van Reeth, Timothy; Sana, Hugues; St-Louis, Nicole; de Oliveira, Alexandre Soares; Todt, Helge; Toonen, Silvia
• 署名单位: University of Amsterdam; Royal Military College - Canada; KU Leuven; European Southern Observatory; Tel Aviv University; University of Bonn; Max Planck Society; National Science Foundation (NSF); University of Potsdam; Universite de Montreal; Universidade do Vale do Paraiba; Consejo Superior de Investigaciones Cientificas (CSIC); CSIC - Centro de Astrobiologia (INTA)
• 刊物名称: SCIENCE
• ISSN/ISSBN: 0036-13701
• DOI: 10.1126/science.ade3293
• 发表日期: 2023-08-18
• 页码: 761-765
• 关键词: wolf-rayet stars; mimes survey; EVOLUTION; CLASSIFICATION; progenitors; supernovae; DISCOVERY; eddington; hd-45166; models

摘要

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.