Imagen de Portada

A Face-on Accretion Disk Geometry Revealed by Millimeter-wave Periodicity in Sgr A$^*$

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Yanagisawa, Kazuki, Oka, Tomoharu, Ariyama, Ryo, Yanagihara, Kazuki, iwata, Yuhei, Takahashi, Mikiya M.
Formato:	Preprint
Publicado:	2025
Materias:	High Energy Astrophysical Phenomena Astrophysics of Galaxies
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

Evidence for Multiple Orbiting Hotspots in the 340 GHz Variability of Sgr A*
por: Yanagisawa, Kazuki, et al.
Publicado: (2026)

Detection of a Molecular Cloud toward the Heartbeating Gamma-ray Source near the Microquasar SS 433
por: Oka, Tomoharu, et al.
Publicado: (2026)

First Mid-infrared Detection and Modeling of a Flare from Sgr A*. II. Mid-IR Spectral Energy Distribution and Millimeter Polarimetry
por: Michail, Joseph M., et al.
Publicado: (2025)

Perturbing AGN Accretion Disks with Stars and Moderately Massive Black Holes: Implications for Changing-Look AGN and Quasi-Periodic Eruptions
por: Dodd, Sierra A., et al.
Publicado: (2025)

Accretion-modified Stars in Accretion Disks of Active Galactic Nuclei: Contribution to AGN disk viscosity
por: Liu, Jun-Rong, et al.
Publicado: (2026)

Universal Radial Scaling of Large-Scale Black Hole Accretion for Magnetically Arrested And Rocking Accretion Disks
por: Lalakos, Aretaios, et al.
Publicado: (2025)

A Therapy Session with Sgr A*
por: Balakrishnan, Mayura, et al.
Publicado: (2026)

Circumbinary Disk Spectra Irradiated by Two Central Accretion Disks in a Binary Black Hole System
por: Lee, Yunewoo, et al.
Publicado: (2024)

Discovery of Quasar Variability and Early Accretion Disk Signatures at Cosmic Dawn
por: Leung, Gene C. K., et al.
Publicado: (2026)

Reverberation Mapping of Lamp-post and Wind Structures in Accretion Thin Disks
por: Chan, James Hung-Hsu, et al.
Publicado: (2024)

Idealized Global Models of Accretion Disks with Strong Toroidal Magnetic Fields
por: Guo, Minghao, et al.
Publicado: (2025)

Short timescale variation in the submillimeter flux of Sagittarius A*
por: Miyoshi, Makoto, et al.
Publicado: (2026)

Eccentric Accretion Disks in Active Galactic Nuclei
por: Deng, Hongping
Publicado: (2025)

Conditions for Changing-Look AGNs from Accretion Disk-Induced Tidal Disruption Events
por: Wang, Yihan, et al.
Publicado: (2024)

The Relationship Between Simulated Sub-Millimeter and Near-Infrared Images of Sagittarius A* from a Magnetically Arrested Black Hole Accretion Flow
por: Grigorian, Arpiar Avetis, et al.
Publicado: (2024)

Disk Instability Model for Quasi-Periodic Eruptions: Investigating Period Dispersion and Peak Temperature
por: Pan, Xin, et al.
Publicado: (2025)

The Effects of Accretion Feedback on Stellar Evolution in AGN Disks
por: Dittmann, Alexander J., et al.
Publicado: (2026)

Deciphering Radio Emissions from Accretion Disk Winds in Radio-Quiet Active Galactic Nuclei
por: Yamada, Tomoya, et al.
Publicado: (2024)

An Eddington Limited Accretion Disk Wind in the narrow line Seyfert 1, PG 1448+273
por: Reeves, J. N., et al.
Publicado: (2024)

Continuum Reverberation Mapping of Accretion Disks Surrounding Supermassive Black Hole Binaries: Observational Signatures
por: Fu, Yi-Xin, et al.
Publicado: (2025)

Parameter study for hot spot trajectories around Sgr$A*$
por: Antonopoulou, Eleni, et al.
Publicado: (2024)

Direct Collapse Accretion Disks Within Dark Matter Halos: Saturation of the Magnetorotational Instability and the Field Expulsion
por: Luo, Yang, et al.
Publicado: (2024)

Strong X-ray Variability of I Zwicky 1: Obscuration from Clumpy Accretion-Disk Winds
por: Huang, Jian, et al.
Publicado: (2026)

Infrared Line Diagnostics Fail to Constrain Sgr A*'s UV Output
por: Balakrishnan, Mayura, et al.
Publicado: (2026)

Multiwavelength Observations of Sgr A*. II. 2019 July 21 and 26
por: Michail, Joseph M., et al.
Publicado: (2024)

Testing the TDE Outflow Model for the Bipolar Sgr A Lobes at the Galactic Center
por: Li, Sida, et al.
Publicado: (2024)

First mid-infrared detection and modeling of a flare from Sgr A*
por: von Fellenberg, Sebastiano D., et al.
Publicado: (2025)

New Evidence for a Flux-independent Spectral Index of Sgr A* in the Near-infrared
por: Paugnat, Hadrien, et al.
Publicado: (2024)

General Relativistic effects and the NIR variability of Sgr A* II: A systematic approach to temporal asymmetry
por: von Fellenberg, Sebastiano D., et al.
Publicado: (2024)

Masers and Broad-Line Mapping Favor Magnetically-Dominated AGN Accretion Disks
por: Hopkins, Philip F., et al.
Publicado: (2026)

Next Generation Accretion Disk Reflection Model: High-Density Plasma Effects
por: Ding, Yuanze, et al.
Publicado: (2024)

Dynamics of recaptures, ejections and mergers of stellar mass binaries over multiple encounters with SgrA*
por: Sersante, Biancamaria, et al.
Publicado: (2025)

Illuminating gravitational wave sources with Sgr A* flares
por: Seoane, Pau Amaro
Publicado: (2025)

Galactic-scale Feeding Reveals Warped Hypermagnetized Multiphase Circumbinary Accretion Around Supermassive Black Hole Binaries
por: Wang, Hai-Yang, et al.
Publicado: (2025)

A Search for Millimeter-Bright Blazars as Astrophysical Neutrino Sources
por: Abbasi, R., et al.
Publicado: (2025)

Compact Accretion Disks in the Aftermath of Tidal Disruption Events: Parameter Inference from Joint X-ray Spectra and UV/Optical Photometry Fitting
por: Guolo, M., et al.
Publicado: (2025)

Polarization of reflected X-ray emission from the Sgr A molecular complex: multiple flares, multiple sources?
por: Khabibullin, Ildar, et al.
Publicado: (2025)

25 years of XMM-Newton observations of the Sgr A complex: 3D distribution and internal structure of the clouds
por: Stel, G., et al.
Publicado: (2025)

Past activity of Sgr A* is unlikely to affect the local cosmic-ray spectrum up to the TeV regime
por: Fournier, Martin, et al.
Publicado: (2024)

Black Hole Spin Estimation with Time-variable Image of M87 During the Flaring State
por: Takahashi, Mikiya M., et al.
Publicado: (2025)