An INTEGRAL overview of High Mass X-ray Binaries: classes or transitions?
Lara Sidoli, Adamantia Paizis (INAF/IASF-Milano, Italy)

TL;DR
This study systematically analyzed INTEGRAL X-ray observations of about 60 High Mass X-ray Binaries over 14 years, revealing their long-term hard X-ray activity and suggesting a continuum between different supergiant binary subclasses.
Contribution
It provides a comprehensive, quantitative characterization of HMXB hard X-ray properties and explores the potential transitional nature between SgHMXBs and SFXTs.
Findings
HMXBs show diverse long-term hard X-ray activity patterns.
Sub-classes of supergiant binaries may form a continuum rather than distinct groups.
Abstract
We analyzed in a systematic way the public INTEGRAL observations spanning from December 2002 to September 2016, to investigate the hard X-ray properties of about 60 High Mass X-ray Binaries (HMXBs). We considered both persistent and transient sources, hosting either a Be star (Be/XRBs) or a blue supergiant companion (SgHMXBs, including Supergiant Fast X-ray Transients, SFXTs), a neutron star or a black hole. INTEGRAL X-ray light curves (18-50 keV), sampled at a bin time of about 2 ks, were extracted for all HMXBs to derive the cumulative distribution of their hard X-ray luminosity, their duty cycle, the range of variability of their hard X-ray luminosity. This allowed us to obtain an overall and quantitative characterization of the long-term hard X-ray activity of the HMXBs in our sample. Putting the phenomenology observed with INTEGRAL into context with other known source properties…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
