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2024ApJ...974..303Z - Astrophys. J., 974, 303 (2024/October-3)

The Bicoherence Analysis of Type-C Quasiperiodic Oscillations in Swift J1727.8-1613.

ZHU H., WANG W. and ZHU Z.

Abstract (from CDS):

We present the results of bicoherence analysis for Swift J1727.8-1613 during its 2023 outburst, using data from Insight-HXMT. Our analysis focused on observations with quasiperiodic oscillations (QPOs) of frequencies greater than 1 Hz, revealing that all of them belong to type-C QPOs. We found a strong correlation between the QPO frequency and the hardness ratio, as well as a linear relationship between the QPO rms and the hardness ratio. The bicoherence analysis revealed a transition from a “web” pattern to a “hypotenuse” pattern in the low-energy (LE) and high-energy (HE) bands. In the bicoherence patterns, there are correlations between horizontal and vertical bicoherence at f1 = f2 = fQPO with count rates. The diagonal structure at f1 + f2 = fQPO becomes more prominent with increasing energy. Additionally, we discovered a new bicoherence pattern in the medium energy band from 10 to 20 keV; the diagonal structure at f1 + f2 = fhar is prominent only in this energy band, which we refer to as the “parallel” pattern. The bicoherence analysis indicates that the source is likely a low-inclination source.

Abstract Copyright: © 2024. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Black hole physics - High energy astrophysics - Stellar accretion disks - X-ray sources - X-ray binary stars

Simbad objects: 6

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