High-Mass X-ray Binaries in the Milky Way: A closer look with INTEGRAL
arXiv:1505.03651 · doi:10.1007/s00159-015-0082-6
Abstract
High-mass X-ray binaries are fundamental in the study of stellar evolution, nucleosynthesis, structure and evolution of galaxies and accretion processes. Hard X-rays observations by INTEGRAL and Swift have broad- ened significantly our understanding in particular for the super-giant systems in the Milky Way, which number has increased by almost a factor of three. INTEGRAL played a crucial role in the discovery, study and understanding of heavily obscured systems and of fast X-ray transients. Most super-giant systems can now be classified in three categories: classical/obscured, eccentric and fast transient. The classical systems feature low eccentricity and variability factor of about 1000, mostly driven by hydrodynamic phenomena occurring on scales larger than the accretion radius. Among them, systems with short orbital periods and close to Roche-Lobe overflow or with slow winds, appear highly obscured. In eccentric systems, the variability amplitude can reach even higher factors, because of the contrast of the wind density along the orbit. Four super-giant systems, featuring fast outbursts, very short orbital periods and anomalously low accretion rates, are not yet understood. Simulations of the accretion processes on relatively large scales have pro- gressed and reproduce parts of the observations. The combined effects of wind clumps, magnetic fields, neutron star rotation and eccentricity ought to be included in future modelling work. Observations with INTEGRAL in combination with other observatories were also important for detecting cyclotron resonant scattering features in spectra of X-ray pulsars, probing their variations and the geometry of the accretion column and emission regions. Finally, the unique characteristics of INTEGRAL and its long life time played a fundamental role for building a complete catalogue of HXMBs, to study the different populations of these systems ...
106 pages, 16 figures, 4 tables
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- A Suzaku X-ray observation of one orbit of the supergiant fast X-ray transient IGR J16479-4514
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- A Comprehensive Study on RXTE & INTEGRAL Observations of the X-ray Pulsar 4U 1907+09
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- The Rich Mid-Infrared Environments of Two Highly-Obscured X-ray Binaries: Spitzer Observations of IGR J16318-4848 and GX 301-2
- Astrophysical parameters of the peculiar X-ray transient IGR J11215-5952
- The XMM-Newton/INTEGRAL monitoring campaign of IGR J16318-4848
- Discovery of a Peculiar Dip from GX 301-2
- The Orbit and Position of the X-ray Pulsar XTE J1855-026 - an Eclipsing Supergiant System
- X-Ray Observation on the Monoceros R2 Star-Forming Region with the Chandra ACIS-I Array
- Near-infrared identification of the counterpart to X1908+075: a new OB-supergiant X-ray binary
- The soft X-ray counterpart of the newly discovered INTEGRAL source IGRJ16195-4945
- Discovering a 5.72 Day Period in the Supergiant Fast X-ray Transient AX J1845.0-0433
- The stellar wind velocity field of HD 77581
- INTEGRAL long-term monitoring of the Supergiant Fast X-ray Transient XTE J1739-302
- 4U 1909+07: a well-hidden pearl
- The INTEGRAL source IGR J16328-4726: a High Mass X-ray Binary from the Beppo SAX era
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- A large spin-up rate measured with INTEGRAL in the High Mass X-ray Binary Pulsar SAXJ2103.5+4545
- AX J1749.1-2733 and AX J1749.2-2725 - the close pair of X-ray pulsars behind the Galactic Center: an optical identification
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