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تسجيل مستخدم جديدFirm Detection of a Cyclotron Resonance Feature with Suzaku in the X-ray Spectrum of GRO J1008-57 during a Giant Outburst in 2012
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We report on the firm detection of a cyclotron resonance scattering feature (CRSF) in the X-ray spectrum of the Be X-ray binary pulsar, GRO J1008-57, achieved by the Suzaku Hard X-ray Detector during a giant outburst which was detected by the MAXI Gas Slit Camera in 2012 November. The Suzaku observation was carried out on 2012 November 20, outburst maximum when the X-ray flux reached $sim 0.45$ Crab in 4-10 keV, which corresponds to a luminosity of $1.1 times 10^{38}$ erg s$^{-1}$ in 0.5--100 keV at 5.8 kpc. The obtained broadband X-ray spectrum from 0.5 keV to 118 keV revealed a significant absorption feature, considered as the fundamental CRSF, at $sim 76$ keV. This unambiguously reconfirm the previously suggested $sim$ 80 keV spectral feature in GRO J1008$-$57. The implied surface magnetic field, $6.6times 10^{12}$ G, is the highest among binary X-ray pulsars from which CRSFs have ever been detected.
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We report on the observation of the accreting pulsar GRO J1008-57 performed by Insight-HXMT at the peak of the sources 2017 outburst. Pulsations are detected with a spin period of 93.283(1) s. The pulse profile shows double peaks at soft X-rays, and
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