activity
20152026
most citedFormation and Evolution of Compact Object Binaries in AGN Disks

389 citations · 1.7k across the 39 of their papers we have counts for

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28 papers · 1 filter

astro-ph.HE2026

Recoil-regulated extreme mass-ratio inspirals in AGN disks

LingQin Xue, Zoltán Haiman, Hiromichi Tagawa +1

Extreme mass-ratio inspirals (EMRIs) are among the primary targets of future space-based gravitational-wave observatories, such as LISA, TianQin, and Taiji. Active galactic nucleus…

astro-ph.HE2026

Properties of black hole mergers in disks of active galactic nuclei

Hiromichi Tagawa, Zoltán Haiman, Bence Kocsis

Ground-based gravitational wave (GW) observatories have detected approximately 200 binary black hole (BH) mergers. The astrophysical origin of these events are debated, with eviden…

astro-ph.HE2026

Electromagnetic Flares from Compact-Object Mergers in AGN Disks: Signatures and Predictions

Hiromichi Tagawa, Zoltán Haiman, Shigeo S. Kimura +2

Accretion disks in active galactic nuclei (AGN) are promising sites for mergers of stellar-mass black holes (BHs) detectable via gravitational waves (GWs). These environments facil…

astro-ph.HE2026

Evidence for a Delayed UV Counterpart to X-ray Quasi-periodic Eruptions in Ansky

Hengxiao Guo, Zhen Yan, Ya-Ping Li +15

X-ray quasi-periodic eruptions (QPEs) represent a novel population of extreme, repeating nuclear transients whose physical origins remain debated. A defining characteristic of QPEs…

astro-ph.HE2025

Gravitational Wave Phase shifts of black hole mergers in AGN Disks

Hiromichi Tagawa, Connar Rowan, János Takátsy +4

Ground-based gravitational wave (GW) detectors have discovered about 200 compact object mergers. The astrophysical origins of these events are highly debated, and it is possible th…

astro-ph.HE2025

Reconstructing the origin of black hole mergers using sparse astrophysical models

V. Gayathri, Giuliano Iorio, Hiromichi Tagawa +8

The astrophysical origin of binary black hole mergers discovered by LIGO and Virgo remains uncertain. Efforts to reconstruct the processes that lead to mergers typically rely on ei…

astro-ph.HE2025★ 22 cited

GW200208_222617 as an eccentric black-hole binary merger: properties and astrophysical implications

Isobel Romero-Shaw, Jakob Stegmann, Hiromichi Tagawa +4

Detecting orbital eccentricity in a stellar-mass black-hole merger would point to a non-isolated formation channel. Eccentric binaries can form in dense stellar environments such a…

astro-ph.HE2025★ 6 cited

Distinguishing the Origin of Eccentric Black Hole Mergers with Gravitational-wave Spin Measurements

Jakob Stegmann, Davide Gerosa, Isobel Romero-Shaw +3

It remains an open question whether the binary black hole mergers observed with gravitational-wave detectors originate from the evolution of isolated massive binary stars or were d…

astro-ph.HE2025★ 6 cited

LVK S241125n: Massive Binary Black Hole Merger Produces Gamma Ray Burst in Active Galactic Nucleus Disk

Shu-Rui Zhang, Yu Wang, Ye-Fei Yuan +6

Recently, the gravitational-wave (GW) event S241125n, detected by LIGO/Virgo/KAGRA (LVK), has been reported to coincide with a candidate detected by Swift-BAT/GUANO and an X-ray ca…

astro-ph.HE2025★ 11 cited

What Determines the Maximum Mass of AGN-assisted Black Hole Mergers?

LingQin Xue, Hiromichi Tagawa, Zoltan Haiman +1

The origin of merging binary black holes detected through gravitational waves remains a fundamental question in astrophysics. While stellar evolution imposes an upper mass limit of…

astro-ph.HE2024

Time-dependent models of AGN disks with radiation from embedded stellar-mass black holes

Marguerite Epstein-Martin, Hiromichi Tagawa, Zoltan Haiman +1

The brightest steady sources of radiation in the universe, active galactic nuclei (AGN), are powered by gas accretion onto a central supermassive black hole (SMBH). The large sizes…

astro-ph.HE2024★ 12 cited

Indication for a compact object next to a LIGO-Virgo binary black hole merger

Shu-Cheng Yang, Wen-Biao Han, Hiromichi Tagawa +2

The astrophysical origin of binary black hole (BBH) mergers remains uncertain, although many events have been observed by the LIGO-Virgo-KAGRA network. Such mergers are potentially…

astro-ph.HE2023★ 2 cited

Shock cooling and breakout emission for optical flares associated with gravitational wave events

Hiromichi Tagawa, Shigeo S. Kimura, Zoltán Haiman +2

The astrophysical origin of stellar-mass black hole (BH) mergers discovered through gravitational waves (GWs) is widely debated. Mergers in the disks of active galactic nuclei (AGN…

astro-ph.HE2023★ 1 cited

High-energy electromagnetic, neutrino, and cosmic-ray emission by stellar-mass black holes in disks of active galactic nuclei

Hiromichi Tagawa, Shigeo S. Kimura, Zoltán Haiman

Some Seyfert galaxies are detected in high-energy gamma rays, but the mechanism and site of gamma-ray emission are unknown. Also, the origins of the cosmic high-energy neutrino and…

astro-ph.HE2023★ 3 cited

Flares from stars crossing active galactic nuclei disks on low-inclination orbits

Hiromichi Tagawa, Zoltán Haiman

The origin of the recently discovered new class of transients, X-ray quasi-periodic eruptions (QPEs), remains a puzzle. Due to their periodicity and association with active galacti…

astro-ph.HE2023★ 27 cited

Observable signatures of stellar-mass black holes in active galactic nuclei

Hiromichi Tagawa, Shigeo S. Kimura, Zoltán Haiman +2

Stellar-mass black holes (BHs) are predicted to be embedded in the disks of active galactic nuclei (AGN) due to gravitational drag and in-situ star formation. However, clear eviden…

astro-ph.HE2023★ 54 cited

Observable signature of merging stellar-mass black holes in active galactic nuclei

Hiromichi Tagawa, Shigeo S. Kimura, Zoltán Haiman +2

The origin of stellar-mass black hole mergers discovered through gravitational waves is being widely debated. Mergers in the disks of active galactic nuclei (AGN) represent a promi…

astro-ph.HE2021★ 50 cited

Can stellar-mass black hole growth disrupt disks of active galactic nuclei? The role of mechanical feedback

Hiromichi Tagawa, Shigeo S. Kimura, Zoltán Haiman +3

Stellar-mass BHs (sBHs) are predicted to be embedded in active galactic nuclei (AGN) disks due to gravitational drag and in-situ star formation. However, we find that due to a high…

astro-ph.HE2021★ 27 cited

Micro Tidal Disruption Events in Active Galactic Nuclei

Y. Yang, I. Bartos, G. Fragione +5

Active galactic nuclei (AGNs) can act as black hole assembly lines, funneling some of the stellar-mass black holes from the vicinity of the galactic center into the inner plane of…

astro-ph.HE2021★ 1 cited

Signatures of Hierarchical Mergers in Black Hole Spin and Mass distribution

Hiromichi Tagawa, Zoltán Haiman, Imre Bartos +2

Recent gravitational wave (GW) observations by LIGO/Virgo show evidence for hierarchical mergers, where the merging BHs are the remnants of previous BH merger events. These events…

astro-ph.HE2021★ 47 cited

Accretion-Induced Collapse of Neutron Stars in the Disks of Active Galactic Nuclei

Rosalba Perna, Hiromichi Tagawa, Zoltan Haiman +1

The disks of active galactic nuclei (AGNs) have emerged as a rich environment for the evolution of stars and their compact remnants. The very dense medium favors rapid accretion, w…

astro-ph.HE2020★ 142 cited

Mass-gap Mergers in Active Galactic Nuclei

Hiromichi Tagawa, Bence Kocsis, Zoltan Haiman +3

The recently discovered gravitational wave sources GW190521 and GW190814 have shown evidence of BH mergers with masses and spins that could be outside of the range expected from is…

astro-ph.HE2020★ 137 cited

Eccentric Black Hole Mergers in Active Galactic Nuclei

Hiromichi Tagawa, Bence Kocsis, Zoltan Haiman +3

The astrophysical origin of gravitational wave (GW) transients is a timely open question in the wake of discoveries by LIGO/Virgo. In active galactic nuclei (AGNs), binaries form a…

astro-ph.HE2020★ 207 cited

AGN as Potential Factories for Eccentric Black Hole Mergers

J. Samsing, I. Bartos, D. J. D'Orazio +6

There is some weak evidence that the black hole merger named GW190521 had a non-zero eccentricity. In addition, the component black holes' masses exceeded the limit predicted by st…