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- W3101160520 abstract "Context . Current models that explain giant (type II) X-ray outbursts in Be/X-ray binaries (BeXB), are based on the idea of highly distorted disks. They are believed to occur when a misaligned and warped disk becomes eccentric, allowing the neutron star to capture a large amount of material. The BeXB 4U 0115+63 underwent two major outbursts in 2015 and 2017. Aims . Our aim is to investigate whether the structural changes in the disk expected during type II outbursts can be detected through optical polarimetry. Methods . We present the first optical polarimetric observations and new optical spectra of the BeXB 4U 0115+63 covering the period 2013–2017. We study in detail the shape of the H α line profile and the polarization parameters before, during, and after the occurrence of a type II X-ray outburst. Results . We find significant changes in polarization degree and polarization angle and highly distorted line profiles during the 2017 X-ray outburst. The degree of polarization decreased by ∼1%, while the polarization angle, which is supposed to be related with the disk orientation, first increased by ∼10° in about two months and then decreased by a similar amount and on a similar timescale once the X-ray activity ceased. Conclusions . We interpret the polarimetric and spectroscopic variability as evidence for the presence of a warped disk." @default.
- W3101160520 created "2020-11-23" @default.
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- W3101160520 date "2018-10-30" @default.
- W3101160520 modified "2023-09-27" @default.
- W3101160520 title "Warped disks during type II outbursts in Be/X-ray binaries: evidence from optical polarimetry" @default.
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- W3101160520 doi "https://doi.org/10.1051/0004-6361/201833649" @default.
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