Evolution of QPOs in GX 339-4 and EXO 1846-031 with Insight-HXMT and NICER
arXiv:2305.18249 · doi:10.3847/1538-4357/ad5a00
Abstract
We conduct a spectral and timing analysis of GX 339-4 and EXO 1846-031 with the aim of studying the evolution of Type-C QPOs with spectral parameters. The high cadence data from Insight-HXMT and NICER allow us to track them. Type-C QPOs appear at the end of low-hard state and/or hard-intermediate state. The results reveal that the QPO frequency is closely related to the inner disk radius and mass accretion rate in the two sources. Such a correlation is nicely consistent with the dynamic frequency model.
arXiv comment14 pages, 15 figures. v2: refereed version
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