Glimpse of the highly obscured HMXB IGR J16318-4848 with Hitomi
Hitomi Collaboration: Felix Aharonian, Hiroki Akamatsu, Fumie Akimoto,, Steven W. Allen, Lorella Angelini, Marc Audard, Hisamitsu Awaki, Magnus, Axelsson, Aya Bamba, Marshall W. Bautz, Roger Blandford, Laura W. Brenneman,, Gregory V. Brown, Esra Bulbul, Edward M. Cackett

TL;DR
This study uses Hitomi's high-resolution X-ray spectroscopy to analyze the obscured high-mass X-ray binary IGR J16318-4848, revealing detailed properties of its reprocessing material and ionization state despite limited photon counts.
Contribution
First high-resolution spectroscopic analysis of IGR J16318-4848 with Hitomi, providing precise measurements of Fe line width and ionization state in a heavily obscured HMXB.
Findings
Fe Kα line width corresponds to 160 km/s velocity
Fe ionization state estimated as Fe I--IV
Confirmed strong absorption with no Compton shoulder
Abstract
We report a Hitomi observation of IGR J16318-4848, a high-mass X-ray binary system with an extremely strong absorption of N_H~10^{24} cm^{-2}. Previous X-ray studies revealed that its spectrum is dominated by strong fluorescence lines of Fe as well as continuum emission. For physical and geometrical insight into the nature of the reprocessing material, we utilize the high spectroscopic resolving power of the X-ray microcalorimeter (the soft X-ray spectrometer; SXS) and the wide-band sensitivity by the soft and hard X-ray imager (SXI and HXI) aboard Hitomi. Even though photon counts are limited due to unintended off-axis pointing, the SXS spectrum resolves Fe K{\alpha_1} and K{\alpha_2} lines and puts strong constraints on the line centroid and width. The line width corresponds to the velocity of 160^{+300}_{-70} km s^{-1}. This represents the most accurate, and smallest, width…
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