X-ray reprocessing in accreting pulsar GX 301-2 observed with Insight-HXMT

Abstract

We investigate the absorption and emission features in observations of GX 301-2 detected with Insight-HXMT/LE in 2017-2019. At different orbital phases, we found prominent Fe Kalpha, Kbeta and Ni Kalpha lines, as well as Compton shoulders and Fe K-shell absorption edges. These features are due to the X-ray reprocessing caused by the interaction between the radiation from the source and surrounding accretion material. According to the ratio of iron lines Kalpha and Kbeta, we infer the accretion material is in a low ionisation state. We find an orbital-dependent local absorption column density, which has a large value and strong variability around the periastron. We explain its variability as a result of inhomogeneities of the accretion environment and/or instabilities of accretion processes. In addition, the variable local column density is correlated with the equivalent width of the iron Kalpha lines throughout the orbit, which suggests that the accretion material near the neutron star is spherically distributed.

10 pages, 5 figures, 2 tables, accepted for publication in MNRAS

References in corpus (6)

• HI4PI: A full-sky HI survey based on EBHIS and GASS
• VLT/UVES spectroscopy of Wray 977, the hypergiant companion to the X-ray pulsar GX301-2
• An XMM-Newton view of FeKα in HMXBs
• Stellar Wind Accretion in GX301-2: Evidence for a High-density Stream
• Orbital phase resolved spectroscopy of GX 301-2 with MAXI
• The spatial distribution of circumstellar material of the wind-fed system GX 301-2

Cited by in corpus (4)

• X-ray polarimetry of the accreting pulsar GX 301-2
• Pulsating iron spectral features in the emission of X-ray pulsar V0332+53
• X-Ray Views of Galactic Accreting Pulsars in High-Mass X-Ray Binaries
• Test the growth models of black hole by jointing LIGO and Insight-HXMT observations