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Accretion torque reversals in GRO J1008-57 revealed by Insight-HXMT
DOI: 10.1016/j.jheap.2021.01.002 Bibcode: 2021JHEAp..30....1W

Wang, W.; Huang, Y.; Wang, C. +92 more

GRO 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 a…

2021 Journal of High Energy Astrophysics
INTEGRAL 15
Redshift evolution of X-ray spectral index of quasars observed by XMM-NEWTON/SDSS
DOI: 10.1016/j.jheap.2021.04.003 Bibcode: 2021JHEAp..31...37S

Misra, R.; Hayman, Z. M.; Shehata, SH. M. +2 more

We study the X-ray spectral evolution of quasars with red-shift using a sample of 1280 quasars constructed by cross-referencing the XMM-Newton 3 XMM - DR 7 and the optical SDSS-DR14 catalogues. The sources were selected to have a minimum detected X-ray counts >600 and which were not affected by high background. The sample redshift distribution …

2021 Journal of High Energy Astrophysics
XMM-Newton 4
A Suzaku study of the low mass X-ray binary Aquila X-1 in the different states
DOI: 10.1016/j.jheap.2021.05.001 Bibcode: 2021JHEAp..31...12A

Abdelbar, Ahmed M.; Beheary, M. M.; Abdelfatah, Ahmed S. +1 more

We present a Suzaku X-ray study for the neutron star low mass X-ray binary Aquila X-1. The observations of the system carried out during three times in 2011 from October 18 to October 24, where the repeated X-ray transient Aquila X-1 was in the rising phase of the outburst. During this period the source was successfully detected in its different s…

2021 Journal of High Energy Astrophysics
Suzaku 2