期刊
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN
卷 66, 期 3, 页码 -出版社
OXFORD UNIV PRESS
DOI: 10.1093/pasj/psu028
关键词
pulsars: individual (GRO J1008-57); stars: magnetic fields; stars: neutron; X-rays: binaries
资金
- Ministry of Education, Culture, Sports, Science and Technology (MEXT) [24340041, 23244024]
- Grants-in-Aid for Scientific Research [23244024, 24103002, 25105507] Funding Source: KAKEN
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 similar to 0.45 Crab in 4-10 keV, which corresponds to a luminosity of 1.1 x 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 similar to 76 keV. This unambiguously reconfirms the previously suggested similar to 80 keV spectral feature in GRO J1008-57. The implied surface magnetic field, 6.6 x 10(12) G, is the highest among binary X-ray pulsars from which CRSFs have ever been detected.
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