Physics
Scientific paper
Jan 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21540408s&link_type=abstract
American Astronomical Society, AAS Meeting #215, #404.08; Bulletin of the American Astronomical Society, Vol. 42, p.226
Physics
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.
Fukumura Keigo
Kazanas Demos
Shrader Chris R.
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