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arxiv: astro-ph/0206490 · v2 · submitted 2002-06-27 · 🌌 astro-ph

Evidence for a 2:3 resonance in Sco X-1 kHz QPOs

M.A. Abramowicz , T. Bulik , M. Bursa , W. Kluzniak This is my paper
classification 🌌 astro-ph
keywords evidencefrequencyqposanchoredapproximatelyblackcandidatesdouble
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We find evidence that the two high frequency QPOs in Sco X-1 are, more often than not, approximately in the 2:3 frequency ratio familiar from studies of black hole candidates (e.g., XTE J1550-564, Remillard et al. 2002). This implies that the double kHz QPO phenomenon in neutron stars has its origin in properties of strong-field gravity and has little to do with the rotation of a stellar surface or any magnetic field structure anchored in the star.

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Cited by 2 Pith papers

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