Long-term Properties of Accretion Disks in X-ray Binaries: II. Stability of Radiation-Driven Warping

Details Long-term Properties of Accretion Disks in X-ray Binaries: II. Stability of Radiation-Driven Warping Long-term Properties of Accretion Disks in X-ray Binaries: II. Stability of Radiation-Driven Warping

2003-04-03

arxiv.org/abs/astro-ph/0304073v1

Mon.Not.Roy.Astron.Soc. 343 (2003) 1213

Astronomy and Astrophysics

Astrophysics

12 pages, 14 figures, Re-submitted to MNRAS after referee's comments

Scientific paper

10.1046/j.1365-8711.2003.06761.x

A significant number of X-ray binaries are now known to exhibit long-term ``superorbital'' periodicities on timescales of $\sim$ 10 - 100 days. Several physical mechanisms have been proposed that give rise to such periodicities, in particular warping and/or precession of the accretion disk. Recent theoretical work predicts the stability to disk warping of X-ray binaries as a function of the mass ratio, binary radius, viscosity and accretion efficiency, and here we examine the constraints that can be placed on such models by current observations. In paper I we used a dynamic power spectrum (DPS) analysis of long-term X-ray datasets (CGRO, RXTE), focusing on the remarkable, smooth variations in the superorbital period exhibited by SMC X-1. Here we use a similar DPS analysis to investigate the stability of the superorbital periodicities in the neutron star X-ray binaries Cyg X-2, LMC X-4 and Her X-1, and thereby confront stability predictions with observation. We find that the period and nature of superorbital variations in these sources is consistent with the predictions of warping theory. We also use a dynamic lightcurve analysis to examine the behaviour of Her X-1 as it enters and leaves the 1999 Anomalous Low State (ALS). This reveals a significant phase shift some 15 cycles before the ALS, which indicates a change in the disk structure or profile leading into the ALS.

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