On the origin of accretion flow photon index–quasi-periodic oscillation frequency (Γ–vQPO) relation

On the origin of accretion flow photon index–quasi-periodic oscillation frequency (Γ–vQPO) relation

Abstract MAXI J1535-571 outburst was dramatic and the accretion flow exhibits spectra-temporal characteristics related to one another. In this study, MAXI J1535-571 data observed by SWIFT/BAT (Swift/Burst Alert Telescope) and MAXI/GSC (Monitor of All-sky X-ray Image/Gas slit camera) was analyzed. Th...

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Bibliographic Details
Main Authors: Ambrose C. Eze, Romanus N. C. Eze, Augustine E. Chukwude, Fidelis Okey Madu
Format: Article
Language:English
Published: Nature Portfolio 2025-04-01
Series:Scientific Reports
Subjects:
MAXI J1535-571
Hard-intermediate state
Accretion flow characteristics
Mass accretion rates
Resonance condition
Photon index–QPO frequency relation
Online Access:https://doi.org/10.1038/s41598-024-83345-z
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https://doi.org/10.1038/s41598-024-83345-z

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