Probing large-scale wind structures in Vela X-1 using off-states with INTEGRAL
L. Sidoli (1), A. Paizis (1), F. Fuerst (2), J.M. Torrejon (3), P., Kretschmar (4), E. Bozzo (5), K. Pottschmidt (6, 7) (1-INAF-IASF Milano,, Italy, 2-Cahill Center, Caltech, USA, 3-University of Alicante, Spain,, 4-ESA/ESAC, Spain, 5-ISDC, Versoix, Switzerland, 6-CRESST UMD

TL;DR
This study analyzes ten years of INTEGRAL data on Vela X-1, revealing asymmetric off-state occurrences near eclipse ingress caused by ionized wind scattering, providing insights into the large-scale wind structure in this high mass X-ray binary.
Contribution
It presents the first systematic analysis of off-state distribution over a decade, linking asymmetries to ionized wind structures in Vela X-1.
Findings
Off-states occur more frequently near eclipse ingress.
Asymmetry in off-state distribution suggests ionized wind scattering.
Decade-long data coverage enabled detection of orbital pattern.
Abstract
Vela X-1 is the prototype of the class of wind-fed accreting pulsars in high mass X-ray binaries hosting a supergiant donor. We have analyzed in a systematic way ten years of INTEGRAL data of Vela X-1 (22-50 keV) and we found that when outside the X-ray eclipse, the source undergoes several luminosity drops where the hard X-rays luminosity goes below 3x10^35 erg/s, becoming undetected by INTEGRAL. These drops in the X-ray flux are usually referred to as "off-states" in the literature. We have investigated the distribution of these off-states along the Vela X-1 ~8.9 d orbit, finding that their orbital occurrence displays an asymmetric distribution, with a higher probability to observe an off-state near the pre-eclipse than during the post-eclipse. This asymmetry can be explained by scattering of hard X-rays in a region of ionized wind, able to reduce the source hard X-ray brightness…
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