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• W2964157219 abstract "SXP 1062 is a Be X-ray binary (BeXB) located in the Small Magellanic Cloud. It hosts a long-period X-ray pulsar and is likely associated with the supernova remnant MCSNR J0127−7332. In this work we present a multiwavelength view on SXP 1062 in different luminosity regimes. We consider monitoring campaigns in optical (OGLE survey) and X-ray (Swift telescope). During these campaigns a tight coincidence of X-ray and optical outbursts is observed. We interpret this as typical Type I outbursts as often detected in BeXBs at periastron passage of the neutron star (NS). To study different X-ray luminosity regimes in depth, during the source quiescence we observed it with XMM–Newton while Chandra observations followed an X-ray outburst. Nearly simultaneously with Chandra observations in X-rays, in optical the RSS/SALT telescope obtained spectra of SXP 1062. On the basis of our multiwavelength campaign we propose a simple scenario where the disc of the Be star is observed face-on, while the orbit of the NS is inclined with respect to the disc. According to the model of quasi-spherical settling accretion our estimation of the magnetic field of the pulsar in SXP 1062 does not require an extremely strong magnetic field at the present time." @default.
• W2964157219 created "2019-07-30" @default.
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• W2964157219 date "2017-12-06" @default.
• W2964157219 modified "2023-10-14" @default.
• W2964157219 title "A multiwavelength study of SXP 1062, the long-period X-ray pulsar associated with a supernova remnant" @default.
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• W2964157219 doi "https://doi.org/10.1093/mnras/stx3127" @default.
• W2964157219 hasPublicationYear "2017" @default.
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