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- W2595750171 abstract "We reanalysed the archival X-ray observations of double system AE Aquarii, obtained using orbital observatories «XMM-Newton» and «Chandra» in 2001 and 2005 respectively. We made an independent timing analysis with two numerical methods. Our result confirmed the presence of 33 s rotational period of white dwarf in the system. In addition, we confirmed that X-ray pulsations with a period of 16.5 s, which were detected in optical and UV ranges, absent in AE Aquarii spectrum. This may mean that the X-ray emission comes from one of the poles of white dwarf surface." @default.
- W2595750171 created "2017-03-23" @default.
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- W2595750171 date "2017-01-01" @default.
- W2595750171 modified "2023-09-25" @default.
- W2595750171 title "Timing analysis of AE Aquarii X-ray observations" @default.
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- W2595750171 doi "https://doi.org/10.1088/1742-6596/798/1/012001" @default.
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