Abstract
The RXTE observations of Scorpius X-1 in 1996–1999 are presented. The properties of its quasi-periodic X-ray oscillations are studied in detail. The results obtained are used for analysis in terms of the transition-layer model (TLM) and the relativistic-precession model (RPM) for a slowly rotating neutron star. Theoretical predictions of the two models are compared and their self-consistency is verified. The tilt of the magnetosphere to the accretion-disk plane, the neutron-star mass, and its angular momentum are determined in terms of the models.
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Translated from Pis'ma v Astronomicheski\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l}\) Zhurnal, Vol. 28, No. 12, 2002, pp. 902–912.
Original Russian Text Copyright © 2002 by Kuznetsov.
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Kuznetsov, S.I. Quasi-periodic X-ray oscillations in the source Scorpius X-1. Astron. Lett. 28, 811–820 (2002). https://doi.org/10.1134/1.1525832
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DOI: https://doi.org/10.1134/1.1525832