Abstract
We consider the kilohertz quasi-periodic oscillations of low-mass X-ray binaries within the Hartle-Thorne spacetime. We show that the interpretation of the epicyclic frequencies of this spacetime with the observed kilohertz quasi-periodic oscillations, within the Relativistic Precession Model, allows us to extract the total mass M, angular momentum J, and quadrupole moment Q of the compact object in a low-mass X-ray binary. We exemplify this fact by analyzing the data of the Z-source GX 5-1. We show that the extracted multipole structure of the compact component of this source deviates from the one expected from a Kerr black hole and instead it points to a neutron star explanation.
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Boshkayev, K., Rueda, J. & Muccino, M. Extracting multipole moments of neutron stars from quasi-periodic oscillations in low mass X-ray binaries. Astron. Rep. 59, 441–446 (2015). https://doi.org/10.1134/S1063772915060050
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DOI: https://doi.org/10.1134/S1063772915060050