Imagen de Portada

Electromagnetic signatures of black hole clusters in the center of super-Eddington galaxies

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Abaroa, Leandro, Romero, Gustavo E.
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 remarkable microquasar S26: a super-Eddington PeVatron?
por: Abaroa, Leandro, 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)

Size matters: are we witnessing super-Eddington accretion in high-redshift black holes from JWST?
por: Lupi, Alessandro, et al.
Publicado: (2024)

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)

Chasing the light: Shadowing, collimation, and the super-Eddington growth of infant black holes in JWST broad-line AGNs
por: Madau, Piero
Publicado: (2025)

Radiation hydrodynamical simulations of super-Eddington mass transfer and black hole growth in close binaries
por: Toyouchi, Daisuke, et al.
Publicado: (2024)

Sustained super-Eddington accretion in high-redshift quasars
por: Lupi, Alessandro, et al.
Publicado: (2023)

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

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

The case for super-Eddington accretion in JWST broad-line AGN during the first billion years
por: Lambrides, Erini, et al.
Publicado: (2024)

Looking for observational signatures of early binary black hole systems
por: Varniere, Peggy, et al.
Publicado: (2026)

How a Klein-Nishina Modified Eddington limited accretion explains rapid black hole growth in the early universe
por: Frangos, Jackson, et al.
Publicado: (2025)

Quasar Main Sequence unfolded by 2.5D FRADO (Natural expression of Eddington ratio, black hole mass, and inclination)
por: Naddaf, M. H., et al.
Publicado: (2025)

Targeted search for eccentric supermassive binary black holes in OJ 287 and nearby galaxy clusters with PPTA DR3
por: Zhao, Shi-Yi, et al.
Publicado: (2026)

X-ray investigation of possible super-Eddington accretion in a radio-loud quasar at $z=6.13$
por: Ighina, L., et al.
Publicado: (2025)

Observing the launch of an Eddington wind in the luminous Seyfert galaxy PG1211+143
por: Pounds, Ken, et al.
Publicado: (2023)

Eddington envelopes: The fate of stars on parabolic orbits tidally disrupted by supermassive black holes
por: Price, Daniel J., et al.
Publicado: (2024)

The relation between black hole spin and molecular gas in massive galaxies
por: Yongyun, Chen, et al.
Publicado: (2024)

Binary black hole mergers from Population III star clusters
por: Mestichelli, Benedetta, et al.
Publicado: (2024)

Seeds to success: growing heavy black holes in dense star clusters
por: Paiella, Lavinia, et al.
Publicado: (2025)

Galactic center G objects as dust-enshrouded stars near the supermassive black hole
por: Zajaček, Michal, et al.
Publicado: (2024)

A candidate supermassive black hole in a gravitationally-lensed galaxy at $z\approx10$
por: Kovacs, Orsolya E., et al.
Publicado: (2024)

Comparing hierarchical black hole mergers in star clusters and active galactic nuclei
por: Li, Guo-Peng, et al.
Publicado: (2022)

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)

Super-Eddington Accretion in Quasars
por: Marziani, P., et al.
Publicado: (2025)

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

Hierarchical binary black hole mergers in globular clusters: mass function and evolution with redshift
por: Torniamenti, Stefano, et al.
Publicado: (2024)

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

Heavy black hole seed survivors in dwarf galaxies: a case study of Leo I
por: Scoggins, Matthew T., 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)

Evidence for gravitational self-lensing of the central supermassive black hole binary in the Seyfert galaxy NGC 1566
por: Kollatschny, Wolfram, 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)

Massive black hole binaries as sources of low-frequency gravitational waves and X-shape radio galaxies
por: Curyło, Małgorzata, et al.
Publicado: (2023)

A unified accretion disc model for supermassive black holes in galaxy formation simulations: method and implementation
por: Koudmani, Sophie, et al.
Publicado: (2023)

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

Jet interaction with galaxy cluster mergers
por: Domínguez-Fernández, Paola, et al.
Publicado: (2024)

Stellar black holes can "stretch'' supermassive black hole accretion disks
por: Zhou, Shuying, et al.
Publicado: (2024)

Imaging fermionic dark matter cores at the center of galaxies
por: Pelle, Joaquin, et al.
Publicado: (2024)

Stellar-mass black holes on the millimetre fundamental plane of black hole accretion
por: Elford, Jacob S., et al.
Publicado: (2026)

MAGICS III. Seeds sink swiftly: nuclear star clusters dramatically accelerate seed black hole mergers
por: Mukherjee, Diptajyoti, et al.
Publicado: (2024)