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20232026
most citedDynamics and spin alignment in massive, gravito-turbulent circumbinary discs around supermassive black hole binaries

13 citations · 36 across the 14 of their papers we have counts for

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8 papers · 1 filter

astro-ph.HE2026

Spin Demographics of Active Supermassive Black Holes: Updated Estimates from X-ray reflection and Future opportunities

Julia M. Sisk-Reynes, Christopher S. Reynolds, James H. Matthews +5

Understanding the growth of supermassive black holes (SMBHs) requires observational constraints on how their angular momentum (or spin) varies with mass, since the relative importa…

astro-ph.HE2026★ 4 cited

Masers and Broad-Line Mapping Favor Magnetically-Dominated AGN Accretion Disks

Philip F. Hopkins, Dalya Baron, Joanna M. Piotrowska

We present a novel and powerful constraint on the physics of supermassive black hole (BH) accretion disks. We show that in the outer disk (radii pc or $\gtrsim 10…

astro-ph.HE2024

Black hole spin evolution across cosmic time from the NewHorizon simulation

Ricarda S. Beckmann, Yohan Dubois, Marta Volonteri +8

Astrophysical black holes (BHs) have two fundamental properties: mass and spin. While the mass-evolution of BHs has been extensively studied, much less work has been done on predic…

astro-ph.HE2023★ 3 cited

The High Energy X-ray Probe (HEX-P): The Circum-nuclear Environment of Growing Supermassive Black Holes

P. G. Boorman, N. Torres-Albà, A. Annuar +32

Ever since the discovery of the first Active Galactic Nuclei (AGN), substantial observational and theoretical effort has been invested into understanding how massive black holes ha…

astro-ph.HE2023★ 3 cited

The High Energy X-ray Probe (HEX-P): Constraining Supermassive Black Hole Growth with Population Spin Measurements

J. M. Piotrowska, J. A. García, D. J. Walton +24

Constraining the primary growth channel of supermassive black holes (SMBH) remains one the most actively debated questions in the context of cosmological structure formation. Owing…

astro-ph.HE2023★ 1 cited

The High Energy X-ray Probe (HEX-P): Probing the physics of the X-ray corona in active galactic nuclei

E. Kammoun, A. M. Lohfink, M. Masterson +28

The hard X-ray emission in active galactic nuclei (AGN) and black hole X-ray binaries is thought to be produced by a hot cloud of electrons referred to as the corona. This emission…

astro-ph.HE2023★ 13 cited

Dynamics and spin alignment in massive, gravito-turbulent circumbinary discs around supermassive black hole binaries

Martin A. Bourne, Davide Fiacconi, Debora Sijacki +2

Parsec-scale separation supermassive black hole binaries in the centre of gas-rich galaxy merger remnants could be surrounded by massive circumbinary discs (CBDs). Black hole mass…

astro-ph.HE2023

Variability as a predictor for the hard-to-soft state transition in GX 339-4

Matteo Lucchini, Marina Ten Have, Jingyi Wang +17

During the outbursts of black hole X-ray binaries (BHXRBs), their accretion flows transition through several states. The source luminosity rises in the hard state, dominated by non…