Discovery of Quasi-Periodic Oscillations in the Recurrent Burst Emission from SGR 1806-20
Ahmed M. El-Mezeini, Alaa I. Ibrahim

TL;DR
This paper reports the detection of quasi-periodic oscillations in recurrent bursts from SGR 1806-20, revealing frequencies close to those in giant flares, which may provide insights into neutron star properties and oscillation origins.
Contribution
It is the first evidence of QPOs in recurrent bursts of SGR 1806-20 at frequencies similar to giant flare QPOs, expanding understanding of neutron star oscillations.
Findings
Detected QPOs at 84, 103, and 648 Hz in recurrent bursts
QPO frequencies are close to those in giant flares
QPOs are statistically significant with confidence ≥ 4.3 σ
Abstract
We present evidence for Quasi-Periodic Oscillations (QPOs) in the recurrent outburst emission from the soft gamma repeater SGR 1806-20 using NASA's Rossi X-ray Timing Explorer (RXTE) observations. By searching a sample of 30 bursts for timing signals at the frequencies of the QPOs discovered in the 2004 December 27 giant flare from the source, we find three QPOs at 84, 103, and 648 Hz in three different bursts. The first two QPOs lie within 1 from the 92 Hz QPO detected in the giant flare. The third QPO lie within 9 from the 625 Hz QPO also detected in the same flare. The detected QPOs are found in bursts with different durations, morphologies, and brightness, and are vindicated by Monte Carlo simulations, which set a lower limit confidence interval . We also find evidence for candidate QPOs at higher frequencies in other bursts with…
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