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arXiv · 2305.12198

Geodesic model complience with the frequencies of the observed X-ray quasi-period oscillations of XTE J1807-294

Radostina Tasheva·Ivan Stefanov
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Abstract

The investigation of the data for quasi-periodic pulsations observed in the X-ray spectra of the accreting millisecond pulsar XTEJ 1807-294 allows some conclusions to be made about its main parameters - mass and angular momentum. Seven different geodesic models - namely RP, RP1, RP2, TP, TP1, WD and TD are applied in attempt to assess their ability to describe the properties of the central neutron star.

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Radostina Tasheva, Ivan Stefanov. 2023-05-20. Geodesic model complience with the frequencies of the observed X-ray quasi-period oscillations of XTE J1807-294. https://arxiv.org/abs/2305.12198

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