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

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...

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Published inarXiv.org
Main Authors Tasheva, Radostina, Stefanov, Ivan
Format Paper
LanguageEnglish
Published Ithaca Cornell University Library, arXiv.org 20.05.2023
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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.
AbstractList 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.
Author Stefanov, Ivan
Tasheva, Radostina
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Snippet 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...
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SubjectTerms Angular momentum
Deposition
Millisecond pulsars
Neutron stars
X ray spectra
Title Geodesic model complience with the frequencies of the observed X-ray quasi-period oscillations of XTE J1807-294
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