Article
Astronomy & Astrophysics
Indu K. Dihingia, Bhargav Vaidya, Christian Fendt
Summary: Variable features in black hole X-ray binaries, such as oscillations in the truncated accretion disc and transient shocks, have been found to have implications on the emission properties of the system.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
A. Ratheesh, F. Tombesi, K. Fukumura, P. Soffitta, E. Costa, D. Kazanas
Summary: The study investigated the origin and geometry of the accretion disc wind in GRS 1915+105 using high-resolution spectroscopy, revealing a possible magnetic origin of the wind and a multiple ionisation component. The observed variability in the line flux between soft and hard states is most likely due to a large increase in the wind density, suggesting an intimate link between accretion and ejection processes in black hole binaries.
ASTRONOMY & ASTROPHYSICS
(2021)
Article
Astronomy & Astrophysics
William Bethune, Henrik Latter
Summary: By studying global magnetohydrodynamic (MHD) models of accretion disks, we find that the gravitational instability (GI) dynamo exhibits global behavior with large-scale amplification, connecting different regions of the disk. This large-scale amplification can be described by a mean-field model that does not rely on conventional alpha-Omega effects.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
Richard Qiu, Angelo Ricarte, Ramesh Narayan, George N. Wong, Andrew Chael, Daniel Palumbo
Summary: Researchers have introduced a new library consisting of 535,194 model images of supermassive black holes and Event Horizon Telescope (EHT) targets Sgr A* and M87*. They used general relativistic radiative transfer calculations and general relativistic magnetohydrodynamics simulations to compute these images. They then trained a random forest machine learning model on various polarimetric observables to infer underlying black hole and accretion flow parameters.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Angelo Ricarte, Richard Qiu, Ramesh Narayan
Summary: Using GRMHD simulations, the study explores the impact of magnetic field geometry on circular polarization images of black hole accretion flows, revealing the stability of circular polarization signs and direct properties of the magnetic field. By decomposing images and identifying light bending effects, novel aspects of helical magnetic field structure on circular polarization images are illustrated.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
G. Marcel, J. Ferreira, P-O Petrucci, S. Barnier, J. Malzac, A. Marino, M. Coriat, M. Clavel, C. Reynolds, J. Neilsen, R. Belmont, S. Corbel
Summary: This paper investigates the spectral evolution and radiative efficiency of transient X-ray binaries. The results show that within the JED-SAD model, a unique pattern in the (in)-R-J plane is followed by all cycles. The study also reveals that the accretion flow in the hard states is always radiatively efficient.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
Chandra B. Singh, Toru Okuda, Ramiz Aktar
Summary: This study investigates two-dimensional low angular momentum flow around a black hole using the resistive magnetohydrodynamic module of PLUTO code. It finds that for flows with lower resistivity, there are quasi-periodic variations in luminosity and shock locations on the equator, while higher resistivity suppresses magnetic activity leading to steady and symmetric flows. These findings shed light on the possibility of explaining long-term flares of Sgr A* in recent observations.
RESEARCH IN ASTRONOMY AND ASTROPHYSICS
(2021)
Article
Astronomy & Astrophysics
A. Raj, C. J. Nixon
Summary: Accretion disks around black holes can become warped and unstable, leading to a dynamic and variable accretion flow. Recent studies have shown that strongly warped disks may break into discrete rings, causing observable fluctuations in the accretion process.
ASTROPHYSICAL JOURNAL
(2021)
Article
Astronomy & Astrophysics
Ramesh Narayan, Andrew Chael, Koushik Chatterjee, Angelo Ricarte, Brandon Curd
Summary: We present the results of nine simulations of radiatively inefficient magnetically arrested discs (MADs) with different black hole spin parameters. Our study finds that the saturated magnetic flux level and jet power of MAD discs strongly depend on the black hole spin. Prograde discs have higher magnetic flux and more powerful jets compared to retrograde discs. Moreover, MADs with spinning black holes launch jets with generalized parabolic profiles, and the width of the jets varies with distance from the black hole according to a power-law function. We also observe a strong correlation between the disc-jet geometry and the dimensionless magnetic flux, with prograde systems displaying thinner equatorial accretion flows near the black hole and wider jets compared to retrograde systems. Additionally, we find different trends in disc variability between prograde and retrograde MADs.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Hai Yang, Feng Yuan, Tom Kwan, Lixin Dai
Summary: This paper investigates the properties of wind and jet launched from a magnetized super-Eddington accretion flow around a supermassive black hole. The simulation data is analyzed using the 'virtual particle trajectory' approach, and the mass flux, velocity, momentum and energy fluxes of wind and jet are obtained. The results show that the mass flux is higher than previous methods suggest, and the momentum flux of wind is larger than that of jet, indicating that wind likely plays a more important role in AGN feedback. The acceleration mechanism of wind and jet is found to be dominated by Lorentz force rather than radiation force.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Chandra B. Singh, Santanu Mondal, David Garofalo
Summary: The study investigates the physical origin of low-frequency quasi-periodic oscillations (LFQPOs) observed in black hole X-ray binaries, considering a minimum number of free parameters, and confirms an anticorrelation between QPO frequency and the location of the shock. Compton cooling is found to be sufficient to explain the observed QPOs.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Samik Mitra, Debaprasad Maity, Indu Kalpa Dihingia, Santabrata Das
Summary: We present a novel approach to study the global structure of steady, axisymmetric, advective, magnetohydrodynamic (MHD) accretion flow around black holes in full general relativity (GR). Considering ideal MHD conditions and relativistic equation of state (REoS), we solve the governing equations to obtain all possible smooth global accretion solutions. We examine the dynamical and thermodynamical properties of accreting matter in terms of the flow parameters, namely energy (epsilon), angular momentum (L), and local magnetic fields. We observe that toroidal component of the magnetic fields generally dominates over radial component at the disc equatorial plane, suggesting the importance of toroidal magnetic field in regulating the disc dynamics. The disc remains mostly gas pressure dominated except at the near horizon region where magnetic fields become indispensable. We calculate the viscosity parameter and examine the scaling relation between alpha and beta, distinguishing two domains along the radial extent of the disc. We discuss the utility of the present formalism in GRMHD simulation studies.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Simone S. Bavera, Tassos Fragos, Emmanouil Zapartas, Enrico Ramirez-Ruiz, Pablo Marchant, Luke Z. Kelley, Michael Zevin, Jeff J. Andrews, Scott Coughlin, Aaron Dotter, Konstantinos Kovlakas, Devina Misra, Juan G. Serra-Perez, Ying Qin, Kyle A. Rocha, Jaime Roman-Garza, Nam H. Tran, Zepei Xing
Summary: The tidal interactions in close binaries can explain the subpopulation of spinning, merging binary black holes and result in long gamma-ray bursts at the time of black-hole formation. This finding allows us to probe the progenitors of binary black-hole mergers well beyond the reach of current gravitational wave observatories.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
Jesse Weder, Christoph Mordasini, Alexandre Emsenhuber
Summary: This study investigates the evolution of large protoplanetary disc populations under the influence of magnetically driven disc winds, internal and external photoevaporation. The simulations show that both strong magnetic torques and weak magnetic winds are necessary to reproduce observed stellar accretion rates. The study also supports the importance of external photoevaporation in disc evolution and its potential influence on planetary formation.
ASTRONOMY & ASTROPHYSICS
(2023)
Article
Astronomy & Astrophysics
Etienne Martel, Geoffroy Lesur
Summary: This study uses numerical simulations to propose that some transition discs (TDs) may be influenced by magnetised disc winds, which could explain their fast accretion and long-lived cavities. The simulations show that material in the cavity is accreted at sonic velocities, while the cavity itself rotates at a high speed due to magnetic braking.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
Aleksey Generozov, Nicholas C. Stone, Brian D. Metzger
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2015)
Article
Astronomy & Astrophysics
A. Generozov, P. Mimica, B. D. Metzger, N. C. Stone, D. Giannios, M. A. Aloy
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2017)
Article
Astronomy & Astrophysics
A. Generozov, N. C. Stone, B. D. Metzger, J. P. Ostriker
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2018)
Article
Astronomy & Astrophysics
A. Yalinewich, R. Sari, A. Generozov, N. C. Stone, B. D. Metzger
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2018)
Article
Astronomy & Astrophysics
Nicholas C. Stone, Aleksey Generozov, Eugene Vasiliev, Brian D. Metzger
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2018)
Article
Astronomy & Astrophysics
Aleksey Generozov
Summary: The Galactic Centre contains young populations, such as the S-stars, which may have originated from tidally disrupted disc binaries, despite their lower mass compared to massive stars in the disc. Possible explanations for this discrepancy include biases in binary disruptions or selective tidal disruptions within the S-star cluster. Tidal disruptions have not significantly affected the mass distribution of the S-stars in recent history.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Alexander Rodriguez, Aleksey Generozov, Ann-Marie Madigan
Summary: The study explores the impact of galactic mergers on eccentric nuclear discs, finding that a second SMBH disrupts the disc stability, while more distant SMBHs can align and stabilize the disc, reducing tidal disruption events.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Alexander Zderic, Maria Tiongco, Angela Collier, Heather Wernke, Aleksey Generozov, Ann-Marie Madigan
Summary: Research shows that axisymmetric disks with eccentric orbits in near-Keplerian potentials are unstable and experience exponential growth in inclination, eventually saturating into a lopsided mode. N-body simulations demonstrate that this apsidal clustering also occurs in the outer solar system's primordial Scattered Disk, with the gravitational influence of giant planets taken into account. The dynamics are explained using Lynden-Bell's mechanism for bar formation in galaxies, and surface density and line-of-sight velocity plots reveal the formation of concentric circles and spiral arms in velocity space during the instability.
ASTRONOMICAL JOURNAL
(2021)
Article
Astronomy & Astrophysics
Aleksey Generozov
ASTROPHYSICAL JOURNAL
(2020)
Article
Astronomy & Astrophysics
P. G. Jonker, N. C. Stone, A. Generozov, S. van Velzen, B. Metzger
ASTROPHYSICAL JOURNAL
(2020)
Article
Astronomy & Astrophysics
Aleksey Generozov, Ann-Marie Madigan
ASTROPHYSICAL JOURNAL
(2020)
Article
Astronomy & Astrophysics
Hayden R. Foote, Aleksey Generozov, Ann-Marie Madigan
ASTROPHYSICAL JOURNAL
(2020)
Article
Astronomy & Astrophysics
Aleksey Generozov, Zoltan Haiman
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2014)