most citedThe Reliability of Accretion Disk Inclination Derived from X-ray Spectroscopy of Active Galaxies

3 citations · 4 across the 6 of their papers we have counts for

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astro-ph.HE2024★ 1 cited

On the Relation between the Inclination Angle of the Accretion Disk and the Broad-line Region in Active Galactic Nuclei

Rong Du, Luis C. Ho, Yuanze Ding +1

Models of active galactic nuclei often invoke a close physical association between the broad-line region and the accretion disk. We evaluate this theoretical expectation by investi…

astro-ph.HE2024

Characterizing the Broadband Reflection Spectrum of MAXI J1803-298 During its 2021 Outburst with NuSTAR and NICER

Oluwashina Adegoke, Javier Garcia, Riley Connors +12

MAXI J1803-298 is a transient black hole candidate discovered in May of 2021 during an outburst that lasted several months. Multiple X-ray observations reveal recurring "dipping" i…

astro-ph.HE2024

Next Generation Accretion Disk Reflection Model: High-Density Plasma Effects

Yuanze Ding, Javier A. García, Timothy R. Kallman +5

Luminous accretion disks around black holes are expected to have densities of cm, which are high enough such that plasma physics effects become important.…

astro-ph.HE2024

Evidence for a nearly orthogonal rotator in GX 301--2 with phase-resolved cyclotron resonant scattering features

Xiao Chen, Yuanze Ding, Wei Wang +8

Cyclotron resonant scattering features (CRSFs) are the absorption features in the X-ray spectra of strongly magnetized accretion neutron stars (NSs), which are probably the most re…

astro-ph.HE2024★ 3 cited

The Reliability of Accretion Disk Inclination Derived from X-ray Spectroscopy of Active Galaxies

Rong Du, Yuanze Ding, Luis C. Ho +1

The inclination angle of substructures in active galaxies gives insights into physical components from scales of the vicinity of the central black hole to the entire host galaxy. W…