pith:IWEL75IG
Revisiting the 2021 Outburst of the BHC MAXI J1803-298 Using NICER, NuSTAR, and Insight-HXMT Data
LFQPOs in MAXI J1803-298 arise from the dynamically evolving inner accretion flow.
arxiv:2605.13232 v1 · 2026-05-13 · astro-ph.HE
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Claims
The combined spectral and timing results support a scenario in which LFQPOs in MAXI J1803-298 arise from the dynamically evolving inner accretion flow.
That the two-component advective flow (TCAF) model accurately captures the accretion geometry and yields an unbiased independent black hole mass estimate from the fitted shock location and flow parameters.
Multi-instrument observations of MAXI J1803-298 link LFQPOs to the evolving inner Comptonizing accretion flow in the hard state, with TCAF modeling yielding a black hole mass estimate.
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| First computed | 2026-05-18T02:44:49.578344Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
4588bff50659913d0013ea5589f39c0d3265ec314502f8ab3c86202cd9649eea
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Canonical record JSON
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