New Insights into Low-frequency QPO Phenomena in X-ray Binaries

Physics

Scientific paper

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Scientific paper

We present our analysis of archival X-ray timing data on four galactic compact objects known to exhibit a variety quasi-periodic oscillations. A time-domain approach, utilizing Autocorrelation Functions (ACFs), as opposed to conventional frequency-domain analyses, is pursued to search for possible fresh insights into the long-standing and unsolved QPO problem. We find three distinct cases in the ACFs: (i) an almost pure oscillatory signal (GRS 1915+105), (ii) a long-lived oscillatory signal (XTE J1550-564) and (XTE J1859+226) and (iii) a rapidly-damped oscillatory signal (Cygnus X-2). While our analysis involves a small number of objects, it appears to imply that there may be fundamental differences leading to these distinct signatures. We describe our analysis and speculate on the possible underlying physics.

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