Imagen de Portada

The relation between black hole spin and molecular gas in massive galaxies

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Yongyun, Chen, Qiusheng, Gu, Junhui, Fan, Xiaoling, Yu, Nan, Ding, Xiaotong, Guo, Dingrong, Xiong
Formato:	Preprint
Publicado:	2024
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

The relation between black hole spin and star formation in massive star-forming galaxies
por: Chen, Yongyun, et al.
Publicado: (2025)

The relation between black hole spin, star formation rate, and black hole mass for supermassive black holes
por: Chen, Yongyun, et al.
Publicado: (2025)

Jets, accretion and spin in supermassive black holes
por: Chen, Yongyun, et al.
Publicado: (2024)

The relation between the optical variability timescale, magnetic field of jets and black hole spin in active galactic nuclei
por: Chen, Yongyun, et al.
Publicado: (2025)

A universal relationship between the variability timescale and black hole mass in black hole jetted and non-jetted accreting systems
por: Chen, Yongyun, et al.
Publicado: (2026)

Observational evidence for a correlation between the magnetic field of jets and star formation rate in host galaxies
por: Chen, Yongyun, et al.
Publicado: (2025)

The cold molecular gas regulates the activity of active galactic nuclei in massive galaxies
por: Chen, Yongyun, et al.
Publicado: (2026)

Characterizing the origins of gamma-ray variability of the jetted active galactic nuclei observed with the Fermi-LAT
por: Chen, Yongyun, et al.
Publicado: (2026)

The fundamental plane of blazars based on the black hole spin-mass energy
por: Zhang, Xu, et al.
Publicado: (2024)

Identifying Compton-thick AGNs in the COSMOS. I. Among X-ray AGNs with Low Photon Counts
por: Guo, Xiaotong, et al.
Publicado: (2025)

A characteristic optical variability time scale in jetted active galactic nuclei: a large gamma-ray emission sample
por: Xiong, Dingrong, et al.
Publicado: (2025)

Evolution of massive black hole in galactic nucleus
por: Inoue, Hajime
Publicado: (2024)

Massive black holes and their galaxies
por: Beckmann, Ricarda S., et al.
Publicado: (2026)

Dynamics and spin alignment in massive, gravito-turbulent circumbinary discs around supermassive black hole binaries
por: Bourne, Martin A., et al.
Publicado: (2023)

On the behaviour of eccentric sub-pc massive black hole binaries embedded in massive discs
por: Franchini, Alessia, et al.
Publicado: (2024)

AT 2021hdr: A candidate tidal disruption of a gas cloud by a binary super massive black hole system
por: Hernández-García, L., et al.
Publicado: (2024)

RABBITS - III. Modelling relativistic accretion discs around spinning black holes in galaxy formation simulations
por: Irodotou, Dimitrios, et al.
Publicado: (2026)

Spin-up and spin distribution of stellar black holes grown by gas accretion in proto-stellar clusters
por: Roupas, Zacharias
Publicado: (2026)

The relationships between AGN power and molecular gas mass within 500 pc of the center of elliptical galaxies
por: Fujita, Yutaka, et al.
Publicado: (2023)

Suppressed accretion onto massive black hole binaries surrounded by thin disks
por: Tiede, Christopher, et al.
Publicado: (2024)

Radiative magnetohydrodynamics simulation of minidisks in equal-mass massive black hole binaries
por: Chan, Chi-Ho, et al.
Publicado: (2025)

Identifying Compton-thick active galactic nuclei in the COSMOS. II. Searching among mid-infrared selected AGNs
por: Guo, Xiaotong, et al.
Publicado: (2026)

Discovery of extreme Quasi-Periodic Eruptions in a newly accreting massive black hole
por: Hernández-García, Lorena, et al.
Publicado: (2025)

How supermassive black holes shape central entropies in galaxy clusters
por: Weinberger, Rainer, et al.
Publicado: (2026)

Electromagnetic signatures of black hole clusters in the center of super-Eddington galaxies
por: Abaroa, Leandro, et al.
Publicado: (2024)

Stars or gas? Constraining the hardening processes of massive black-hole binaries with LISA
por: Spadaro, Alice, et al.
Publicado: (2024)

X-ray properties of reverberation-mapped AGNs with super-Eddington accreting massive black holes
por: Maithil, Jaya, et al.
Publicado: (2024)

Neural Networks unveiling the properties of gravitational wave background from massive black hole binaries
por: Bonetti, Matteo, et al.
Publicado: (2023)

Optically thick winds of very massive stars suppress intermediate-mass black hole formation
por: Torniamenti, Stefano, et al.
Publicado: (2025)

Black holes regulate cool gas accretion in massive galaxies
por: Wang, Tao, et al.
Publicado: (2023)

On the origin of a possible hard VHE spectrum from M87 discovered by LHAASO
por: Xue, Rui, et al.
Publicado: (2025)

A novel sub-grid model for super-Eddington accretion of spinning black holes in galaxy-scale simulations
por: Kao, Wei-Bo, et al.
Publicado: (2025)

Identifying massive black hole binaries via light curve variability in optical time-domain surveys
por: Chiesa, Alfredo, et al.
Publicado: (2025)

X-ray AGN in Boötes: The lack of growth of the most massive black holes since z=4
por: Guetzoyan, Paloma, et al.
Publicado: (2024)

JWST MIRI/MRS observations of hot molecular gas in an AGN host galaxy at Cosmic Noon
por: Kakkad, D., et al.
Publicado: (2025)

Searching for unresolved massive black hole pairs through AGN photometric variability
por: Bertassi, Lorenzo, et al.
Publicado: (2026)

Stellar distributions around supermassive black holes in gas-rich nuclear star clusters
por: Rozner, Mor, et al.
Publicado: (2025)

Stellar-mass black holes in young massive and open stellar clusters -- VI. Role of external galactic field
por: Banerjee, Sambaran
Publicado: (2025)

Constraints on dynamically-formed massive black holes in Little Red Dots from X-ray non-detections
por: Liempi, M., et al.
Publicado: (2026)

Accretion mediated spin-eccentricity correlations in LISA massive black hole binaries
por: Garg, Mudit, et al.
Publicado: (2024)