Self-Consistent Disk-Reflection Analysis of the Black-Hole Candidate X-ray Binary MAXI J1813-095 with NICER, Swift, Chandra, and NuSTAR
Santiago Ubach, James F. Steiner, Jiachen Jiang, Javier Garcia, Riley, M.T. Connors, Guglielmo Mastroserio, Ye Feng, John A. Tomsick

TL;DR
This study analyzes the black-hole candidate MAXI J1813-095 during its 2018 outburst using multi-instrument X-ray data, revealing a relativistic iron line, a possibly truncated disk, and a high reflection fraction, advancing understanding of accretion physics.
Contribution
It introduces a self-consistent spectral modeling approach coupling disk, Comptonization, and reflection components, with a focus on the reflection fraction and disk geometry in MAXI J1813-095.
Findings
Relativistic iron line detected at ~6.5 keV.
Inner disk radius estimated at ~2 Rg, consistent with a slightly truncated disk.
Reflection fraction found to be of order unity, higher than previous estimates.
Abstract
We present our analysis of MAXI J1813-095 during its hard state ``stalled'' outburst in 2018. This self-consistent analysis has been carried out using \NICER, \Swift, \Chandra, and {\NuSTAR} throughout seven observations of MAXI J1813-095. We find a relativistic iron line at 6.5 keV from the inner region of the accretion disk. Our results are consistent with a slightly truncated disk or non-truncated disk for an inner radius of 2 and minimum spin of 0.7 with a best value of , assuming reaches the innermost stable circular orbit at 1\% . We analyzed MAXI J1813-095 over its outburst employing a spectral model which self-consistently couples the seed disk photons to the Comptonization and reflection components, also inclusive of reflection Comptonization. The unique aspect of this work is…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Mechanics and Biomechanics Studies
