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Accretion torque reversals in GRO J1008-57 revealed by Insight-HXMT
Wang, W.; Tang, Y. M.; Tuo, Y. L.; Epili, P. R.; Zhang, S. N.; Song, L. M.; Lu, F. J.; Qu, J. L.; Zhang, S.; Ge, M. Y.; Huang, Y.; Li, B.; Bu, Q. C.; Cai, C.; Cao, X. L.; Chang, Z.; Chen, L.; Chen, T. X.; Chen, Y. B.; Chen, Y.; Chen, Y. P.; Cui, W. W.; Du, Y. Y.; Gao, G. H.; Gao, H.; Gu, Y. D.; Guan, J.; Guo, C. C.; Han, D. W.; Huo, J.; Jia, S. M.; Jiang, W. C.; Jin, J.; Kong, L. D.; Li, C. K.; Li, G.; Li, T. P.; Li, W.; Li, X.; Li, X. B.; Li, X. F.; Li, Z. W.; Liang, X. H.; Liao, J. Y.; Liu, B. S.; Liu, C. Z.; Liu, H. X.; Liu, H. W.; Lu, X. F.; Luo, Q.; Luo, T.; Ma, R. C.; Ma, X.; Meng, B.; Nang, Y.; Nie, J. Y.; Ou, G.; Ren, X. Q.; Sai, N.; Song, X. Y.; Sun, L.; Tao, L.; Wang, C.; Wang, L. J.; Wang, P. J.; Wang, W. S.; Wang, Y. S.; Wen, X. Y.; Wu, B. Y.; Wu, B. B.; Wu, M.; Xiao, G. C.; Xiao, S.; Xiong, S. L.; Xu, Y. P.; Yang, R. J.; Yang, S.; Yang, J. J.; Yang, Y. J.; Yi, B. B.; Yin, Q. Q.; You, Y.; Zhang, F.; Zhang, H. M.; Zhang, J.; Zhang, P.; Zhang, W.; Zhang, W. C.; Zhang, Y. F.; Zhang, Y. H.; Zhao, H. S.; Zhao, X. F.; Zheng, S. J.; Zheng, Y. G.; Zhou, D. K.
Source PublicationJournal of High Energy Astrophysics
AbstractGRO J1008-57, as a Be/X-ray transient pulsar, is considered to have the highest magnetic field in known neutron star X-ray binary systems. Observational data of the X-ray outbursts in GRO J1008-57 from 2017 to 2020 were collected by the Insight-HXMT satellite. In this work, the spin period of the neutron star in GRO J1008-57 was determined to be about 93.28 seconds in August 2017, 93.22 seconds in February 2018, 93.25 seconds in June 2019 and 93.14 seconds in June 2020. GRO J1008-57 evolved in the spin-up process with a mean rate of - (2.10 ± 0.05) ×10-4 s/d from 2009 - 2018, and turned into a spin down process with a rate of (6.7 ± 0.6) ×10-5 s/d from Feb 2018 to June 2019. During the type II outburst of 2020, GRO J1008-57 had the spin-up torque again. During the torque reversals, the pulse profiles and continuum X-ray spectra did not change significantly, and the cyclotron resonant scattering feature around 80 keV was only detected during the outbursts in 2017 and 2020. Based on the observed mean spin-up rate, we estimated the inner accretion disk radius in GRO J1008-57 (about 1 - 2 times of the Alfvén radius) by comparing different accretion torque models of magnetic neutron stars. During the spin-down process, the magnetic torque should dominate over the matter accreting inflow torque, and we constrained the surface dipole magnetic field B ≥ 6 ×1012 G for the neutron star in GRO J1008-57, which is consistent with the magnetic field strength obtained by cyclotron line centroid energy.
WOS IDWOS:000657475900001
ADS Bibcode2021JHEAp..30....1W
ADS URLhttps://ui.adsabs.harvard.edu/abs/2021JHEAp..30....1W
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Cited Times:4 [ADS]
Document Type期刊论文
Recommended Citation
GB/T 7714
Wang, W.,Tang, Y. M.,Tuo, Y. L.,et al. Accretion torque reversals in GRO J1008-57 revealed by Insight-HXMT[J]. Journal of High Energy Astrophysics,2021,30:1.
APA Wang, W..,Tang, Y. M..,Tuo, Y. L..,Epili, P. R..,Zhang, S. N..,...&Zhou, D. K..(2021).Accretion torque reversals in GRO J1008-57 revealed by Insight-HXMT.Journal of High Energy Astrophysics,30,1.
MLA Wang, W.,et al."Accretion torque reversals in GRO J1008-57 revealed by Insight-HXMT".Journal of High Energy Astrophysics 30(2021):1.
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