activity
20182026
most cited1ES 1927+654: An AGN Caught Changing Look on a Timescale of Months

193 citations · 349 across the 29 of their papers we have counts for

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8 papers · 1 filter

astro-ph.HE2026

Spectral Appearance of Self-gravitating Disks Powered by Stellar Objects: Universal Effective Temperature in the Optical Continuum and Application to Little Red Dots

Yi-Xian Chen, Hanpu Liu, Ruancun Li +6

We revisit the spectral appearance of extended self-gravitating accretion disks surrounding compact central objects such as supermassive black holes. Using dust-poor opacities, we…

astro-ph.HE2025★ 8 cited

The Average Soft X-ray Spectra of eROSITA Active Galactic Nuclei

Shi-Jiang Chen, Johannes Buchner, Teng Liu +16

Context. AGNs are strong X-ray emitters shaped by disk-corona interactions. The soft excess (0.5-2.0 keV) reveals key information about the "warm corona" bridging the disk and hot…

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

A Two-zone Accretion Disk in the Changing-look Active Galactic Nucleus 1ES 1927+654: Physical Implications for Tidal Disruption Events and Super-Eddington Accretion

Ruancun Li, Luis C. Ho, Claudio Ricci +1

The properties of slim accretion disks, while crucial for our understanding of black hole growth, have yet to be studied extensively observationally. We analyze the multi-epoch bro…

astro-ph.HE2024★ 1 cited

The Interplay between the Disk and Corona of the Changing-look Active Galactic Nucleus 1ES 1927+654

Ruancun Li, Claudio Ricci, Luis C. Ho +4

Time-domain studies of active galactic nuclei (AGNs) offer a powerful tool for understanding black hole accretion physics. Prior to the optical outburst on 23 December 2017, 1ES 19…

astro-ph.HE2024★ 1 cited

Sub-relativistic Outflow and Hours-Timescale Large-amplitude X-ray Dips during Super-Eddington Accretion onto a Low-mass Massive Black Hole in the Tidal Disruption Event AT2022lri

Yuhan Yao, Muryel Guolo, Francesco Tombesi +32

We present the tidal disruption event (TDE) AT2022lri, hosted in a nearby ( Mpc) quiescent galaxy with a low-mass massive black hole ($10^4\,M_\odot < M_{\rm BH} < 10…

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…

astro-ph.HE2022★ 22 cited

Systematic Broad-band X-ray Study of super-Eddington Accretion onto Supermassive Black Holes. I. X-ray Continuum

Alessia Tortosa, Claudio Ricci, Luis C. Ho +6

We present the first systematic broad-band X-ray study of super-Eddington accretion onto SMBHs with simultaneous {\it NuSTAR} and {\it XMM-Newton} or {\it Swift}/XRT observations o…