activity
20082026
most citedMassive black hole binary mergers within sub-pc scale gas discs

402 citations · 770 across the 17 of their papers we have counts for

collaborators

18 papers

astro-ph.HE2026

Alignment-driven binary evolution in warped circumbinary discs: 3D moving-mesh hydrodynamics of eccentric and inclined binaries

Lazaros Souvaitzis, Magdalena Siwek, Jorge Cuadra

We present three-dimensional moving-mesh hydrodynamical simulations (\arepo{}) of equal-mass binaries in circumbinary discs, spanning binary eccentricity () an…

astro-ph.GA2026

Interacting stellar winds feeding Sgr A*: from the system of mass-losing stars to the binary IRS 16SW

Diego Calderón, Jorge Cuadra, Christopher M. P. Russell +3

The discovery of cold structures around Sgr A* has challenged our understanding of the gas dynamics and thermodynamic state of the plasma in its vicinity. This work aims to constra…

astro-ph.GA2026

Superdiffusion at the Galactic Centre

Pau Amaro Seoane, Kostas Tzanavaris, Reinhard Genzel +14

Tracking S-star cluster orbits around Sgr A* calibrates orbital transport models for space-borne gravitational wave detectors. Standard kinetic theories model this cluster via loca…

astro-ph.GA2026

Stellar rotation of S301 as a macroscopic gyroscope to test general relativity

Pau Amaro Seoane, Xian Chen, Alejandro Torres-Orjuela +16

Stellar trajectories around the Galactic Center provide a testing environment for general relativity. The intrinsic rotation of these stars evolves under covariant transport in cur…

astro-ph.GA2026

S301 and friends: Measuring the spin of Sgr A*

T. Piran, P. Amaro-Seoane, B. Aytac +15

The discovery of S301 (GRAVITY Collaboration et al., 2026) with pericenter distance rp= 280rg and eccentricity e=0.9825, opens the prospect of measuring the spin parameter of Sgr A…

astro-ph.GA2025★ 1 cited

The gas streamer G1-2-3 in the Galactic Center

S. Gillessen, F. Eisenhauer, J. Cuadra +61

The black hole in the Galactic Center, Sgr A*, is prototypical for ultra-low-fed galactic nuclei. The discovery of a hand-full of gas clumps in the realm of a few Earth masses in i…

astro-ph.GA2025★ 1 cited

Tidal phenomena in the Galactic Center: The curious case of X7

Wasif Shaqil, Diego Calderón, Stephan Rosswog +5

Several enigmatic dusty sources have been detected in the central parsec of the Galactic Center. Among them is X7, located at only 0.02 pc from the central super-massive blac…

astro-ph.GA2024★ 9 cited

The formation and stability of a cold disc made out of stellar winds in the Galactic Centre

Diego Calderón, Jorge Cuadra, Christopher M. P. Russell +3

The reported discovery of a cold (~10 K) disc-like structure within 0.005 pc around the super-massive black hole at the centre of the Milky Way, Sgr A*, has challenged our unde…

astro-ph.HE2024

Multistructured accretion flow of Sgr A* II: Signatures of a Cool Accretion Disk in Hydrodynamic Simulations of Stellar Winds

Mayura Balakrishnan, Christopher M. P. Russell, Lia Corrales +8

Hydrodynamic simulations of the stellar winds from Wolf-Rayet stars within the Galactic Center can provide predictions for the X-ray spectrum of supermassive black hole Sgr A*. Her…

astro-ph.HE2024★ 40 cited

Long-term Evolution of Binary Orbits Induced by Circumbinary Disks

Ruggero Valli, Christopher Tiede, Alejandro Vigna-Gómez +6

Circumbinary disks are found in a variety of astrophysical scenarios, spanning binary star formation to accreting supermassive black hole binaries. The interaction with a circumbin…

astro-ph.GA2015★ 34 cited

Clump formation through colliding stellar winds in the Galactic Centre

D. Calderón, A. Ballone, J. Cuadra +3

The gas cloud G2 is currently being tidally disrupted by the Galactic Centre super-massive black hole, Sgr A*. The region around the black hole is populated by Wolf-Rayet…

astro-ph.HE2015★ 35 cited

Infalling clouds onto super-massive black hole binaries - I. Formation of discs, accretion and gas dynamics

F. G. Goicovic, J. Cuadra, A. Sesana +3

There is compelling evidence that most -if not all- galaxies harbour a super-massive black hole (SMBH) at their nucleus, hence binaries of these massive objects are an inevitable p…

astro-ph.SR2015★ 130 cited

Accretion kinematics through the warped transition disk in HD142527 from resolved CO(6-5) observations

Simon Casassus, Sebastian Marino, Sebastian Perez +10

The finding of residual gas in the large central cavity of the HD142527 disk motivates questions on the origin of its non-Keplerian kinematics, and possible connections with planet…

astro-ph.GA2015★ 28 cited

Super massive black holes in star forming gaseous circumnuclear discs

Luciano del Valle, Andres Escala, Cristian Maureira-Fredes +3

Using N-body/SPH simulations we study the evolution of the separation of a pair of SMBHs embedded in a star forming circumnuclear disk (CND). This type of disk is expected to be fo…

astro-ph.GA2014★ 4 cited

Tidal disruptions in circumbinary disks. II: Observational signatures in the reverberation spectra

Patrick Brem, Jorge Cuadra, Pau Amaro-Seoane +1

Supermassive Binary Black Holes (SMBBHs) with sub-pc separations form in the course of galaxy mergers, if both galaxies harbour massive black holes. Clear observational evidence fo…

astro-ph.GA2013

Observations of the gas cloud G2 in the Galactic Center

Stefan Gillessen, Reinhard Genzel, Tobias K. Fritz +6

In 2011, we discovered a compact gas cloud ("G2") with roughly three Earth masses that is falling on a near-radial orbit toward the massive black hole in the Galactic Center. The o…

astro-ph.GA2012★ 86 cited

New observations of the gas cloud G2 in the Galactic Center

S. Gillessen, R. Genzel, T. K. Fritz +6

We present new observations of the recently discovered gas cloud G2 currently falling towards the massive black hole in the Galactic Center. The new data confirm that G2 is on a hi…

astro-ph2008★ 402 cited

Massive black hole binary mergers within sub-pc scale gas discs

J. Cuadra, P. J. Armitage, R. D. Alexander +1

[ABRIDGED] We study supermassive black hole binary mergers driven by angular momentum loss to small-scale gas discs. Such binaries form after major galaxy mergers, but their fate i…