The Growth of the Central Black Holes in Quasi-stars
Fuente:
arXiv
Guardado en:
| Autores principales: | Hassan, Jake, Perna, Rosalba, Cantiello, Matteo, Armitage, Philip, Begelman, Mitchell, Ryu, Taeho |
|---|---|
| Formato: | Preprint |
| Publicado: |
2025
|
| Materias: | |
| Acceso en línea: | |
| Etiquetas: |
Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
|
Ejemplares similares
Pulsational Instability of Quasi-Stars: Interpreting the Variability of Little Red Dots
por: Cantiello, Matteo, et al.
Publicado: (2025)
por: Cantiello, Matteo, et al.
Publicado: (2025)
Tidal Disruption Encores
por: Ryu, Taeho, et al.
Publicado: (2024)
por: Ryu, Taeho, et al.
Publicado: (2024)
Quasi-stars as a Means of Rapid Black Hole Growth in the Early Universe
por: Coughlin, Eric R., et al.
Publicado: (2024)
por: Coughlin, Eric R., et al.
Publicado: (2024)
Spectral Evolution of Rotating Population III Stars
por: Hassan, Jake, et al.
Publicado: (2025)
por: Hassan, Jake, et al.
Publicado: (2025)
Delayed emission from luminous blue optical transients in black-hole binary systems
por: Lazzati, Davide, et al.
Publicado: (2024)
por: Lazzati, Davide, et al.
Publicado: (2024)
Blue straggler stars
por: Wang, Chen, et al.
Publicado: (2024)
por: Wang, Chen, et al.
Publicado: (2024)
Mapping the Outcomes of Stellar Evolution in the Disks of Active Galactic Nuclei
por: Fabj, Gaia, et al.
Publicado: (2024)
por: Fabj, Gaia, et al.
Publicado: (2024)
Light curves and spectra for stellar collisions between main-sequence stars in galactic nuclei
por: Ryu, Taeho, et al.
Publicado: (2025)
por: Ryu, Taeho, et al.
Publicado: (2025)
A simple model of globally magnetized accretion discs
por: Begelman, Mitchell C.
Publicado: (2024)
por: Begelman, Mitchell C.
Publicado: (2024)
Micro-turbulence across the Hertzsprung-Russell diagram. Observational constrains for stars in the MW
por: Markova, N., et al.
Publicado: (2025)
por: Markova, N., et al.
Publicado: (2025)
The collision and merger products of stars do not look alike: A magnetohydrodynamics comparison
por: Vynatheya, Pavan, et al.
Publicado: (2025)
por: Vynatheya, Pavan, et al.
Publicado: (2025)
Follow the Mass -- A Concordance Picture of Tidal Disruption Events
por: Krolik, Julian, et al.
Publicado: (2024)
por: Krolik, Julian, et al.
Publicado: (2024)
Floating binary planets from ejections during close stellar encounters
por: Wang, Yihan, et al.
Publicado: (2023)
por: Wang, Yihan, et al.
Publicado: (2023)
She's Got Her Mother's Hair: Unveiling the Origin of Black Hole Magnetic Fields through Stellar to Collapsar Simulations
por: Gottlieb, Ore, et al.
Publicado: (2024)
por: Gottlieb, Ore, et al.
Publicado: (2024)
Simulating the tidal disruption of stars by stellar-mass black holes using moving-mesh hydrodynamics
por: Vynatheya, Pavan, et al.
Publicado: (2023)
por: Vynatheya, Pavan, et al.
Publicado: (2023)
Understanding the impact of binary mass transfer in the accretor's measurable parameters
por: Vilaxa-Campos, Magdalena, et al.
Publicado: (2026)
por: Vilaxa-Campos, Magdalena, et al.
Publicado: (2026)
A Semi-Analytical Model for Stellar Evolution in AGN Disks
por: Dittmann, Alexander J., et al.
Publicado: (2024)
por: Dittmann, Alexander J., et al.
Publicado: (2024)
The Effects of Accretion Feedback on Stellar Evolution in AGN Disks
por: Dittmann, Alexander J., et al.
Publicado: (2026)
por: Dittmann, Alexander J., et al.
Publicado: (2026)
Asymmetrical thermonuclear supernovae triggered by the tidal disruption of white dwarfs
por: Vynatheya, Pavan, et al.
Publicado: (2026)
por: Vynatheya, Pavan, et al.
Publicado: (2026)
On the Missing Red Giants near the Galactic Center
por: Kim, Taeho, et al.
Publicado: (2026)
por: Kim, Taeho, et al.
Publicado: (2026)
Non-conservative Mass Transfer as a Formation Channel for Gaia Black Hole System
por: Olejak, Aleksandra, et al.
Publicado: (2025)
por: Olejak, Aleksandra, et al.
Publicado: (2025)
Predicting Stellar Parameters of Massive Stars from Light Curves with Machine Learning
por: Zhang, Rachel C., et al.
Publicado: (2025)
por: Zhang, Rachel C., et al.
Publicado: (2025)
Evolution of Extremely Soft Binaries in Dense Star Clusters: On the Jupiter Mass Binary Objects
por: Wang, Yihan, et al.
Publicado: (2024)
por: Wang, Yihan, et al.
Publicado: (2024)
A Model for Eruptive Mass Loss in Massive Stars
por: Cheng, Shelley J., et al.
Publicado: (2024)
por: Cheng, Shelley J., et al.
Publicado: (2024)
Type IIb Supernova Progenitors in 3D: Variability and Episodic Mass Loss revealed by Radiation-Hydrodynamics Simulations
por: Goldberg, Jared A., et al.
Publicado: (2025)
por: Goldberg, Jared A., et al.
Publicado: (2025)
Centrally concentrated star formation in young clusters
por: Assilkhan, Adilkhan, et al.
Publicado: (2025)
por: Assilkhan, Adilkhan, et al.
Publicado: (2025)
Central-star extinctions towards planetary nebulae
por: Csukai, Alexander, et al.
Publicado: (2025)
por: Csukai, Alexander, et al.
Publicado: (2025)
Repeating partial disruptions and two-body relaxation
por: Broggi, Luca, et al.
Publicado: (2024)
por: Broggi, Luca, et al.
Publicado: (2024)
Collisions of red giants in galactic nuclei
por: Ryu, Taeho, et al.
Publicado: (2023)
por: Ryu, Taeho, et al.
Publicado: (2023)
Magnetic Field Amplification during Stellar Collisions between Low-Mass Stars
por: Ryu, Taeho, et al.
Publicado: (2024)
por: Ryu, Taeho, et al.
Publicado: (2024)
On the orbital evolution of binaries with polar circumbinary disks
por: Chen, Cheng, et al.
Publicado: (2026)
por: Chen, Cheng, et al.
Publicado: (2026)
Magnetic Fields or Overstable Convective Modes in HR 7495: Exploring the Underlying Causes of the Spike in the 'Hump & Spike' Features
por: Antoci, V., et al.
Publicado: (2025)
por: Antoci, V., et al.
Publicado: (2025)
Inflated hot Jupiters: Inferring average atmospheric velocity via Ohmic models coupled with internal dynamo evolution
por: Viganò, Daniele, et al.
Publicado: (2025)
por: Viganò, Daniele, et al.
Publicado: (2025)
Thermal-timescale accretion does not always yield critical rotation in mass gainers
por: Wang, Chen, et al.
Publicado: (2026)
por: Wang, Chen, et al.
Publicado: (2026)
Hot Jupiter engulfment by a red giant in 3D hydrodynamics
por: Lau, Mike Y. M., et al.
Publicado: (2022)
por: Lau, Mike Y. M., et al.
Publicado: (2022)
MESA Isochrones and Stellar Tracks. II. Models with alpha-enhanced chemical composition
por: Dotter, A, et al.
Publicado: (2026)
por: Dotter, A, et al.
Publicado: (2026)
BlackGEM observations of compact pulsating stars: Mode identification for the DOV PG 1159-035 using multi-colour photometry
por: Ranaivomanana, P., et al.
Publicado: (2026)
por: Ranaivomanana, P., et al.
Publicado: (2026)
Circumplanetary Disks are Rare around Planets at Large Orbital Radii: A Parameter Survey of Flow Morphology around Giant Planets
por: Sagynbayeva, Sabina, et al.
Publicado: (2024)
por: Sagynbayeva, Sabina, et al.
Publicado: (2024)
Tidal Disruption Events from three-body scatterings and eccentricity pumping in the disks of Active Galactic Nuclei
por: Prasad, Chaitanya, et al.
Publicado: (2023)
por: Prasad, Chaitanya, et al.
Publicado: (2023)
Identifying Flare Locations Through Exoplanet Transit Occultations
por: Armitage, Tayt, et al.
Publicado: (2025)
por: Armitage, Tayt, et al.
Publicado: (2025)
Ejemplares similares
-
Pulsational Instability of Quasi-Stars: Interpreting the Variability of Little Red Dots
por: Cantiello, Matteo, et al.
Publicado: (2025) -
Tidal Disruption Encores
por: Ryu, Taeho, et al.
Publicado: (2024) -
Quasi-stars as a Means of Rapid Black Hole Growth in the Early Universe
por: Coughlin, Eric R., et al.
Publicado: (2024) -
Spectral Evolution of Rotating Population III Stars
por: Hassan, Jake, et al.
Publicado: (2025) -
Delayed emission from luminous blue optical transients in black-hole binary systems
por: Lazzati, Davide, et al.
Publicado: (2024)