Imagen de Portada

A framework for modelling Population III stars in cosmological simulations

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Saha, Bipradeep, Kannan, Rahul, Mirouh, Giovanni M.
Formato:	Preprint
Publicado:	2026
Materias:	Astrophysics of Galaxies
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

Quantifying the impact of AGN feedback on the large-scale matter distribution using two- and three-point statistics
por: Saha, Bipradeep, et al.
Publicado: (2024)

The THESAN-ZOOM project: Population III star formation continues until the end of reionization
por: Zier, Oliver, et al.
Publicado: (2025)

A model for star formation in cosmological simulations of galaxy formation
por: Lozano, Ezequiel, et al.
Publicado: (2021)

Enhanced sub-resolution star formation models in cosmological simulations
por: Lozano, Ezequiel, et al.
Publicado: (2025)

Where are the Population III star relics in the simulated Milky Way analogues?
por: Yang, Hang, et al.
Publicado: (2025)

Investigating cosmic strings using large-volume hydrodynamical simulations in the context of JWST's massive UV-bright galaxies
por: Koehler, Sonja M., et al.
Publicado: (2024)

SIEGE III: The formation of dense stellar clusters in sub-parsec resolution cosmological simulations with individual star feedback
por: Calura, F., et al.
Publicado: (2024)

Applying a star formation model calibrated on high-resolution interstellar medium simulations to cosmological simulations of galaxy formation
por: Burger, Jan D., et al.
Publicado: (2025)

RIGEL: Feedback-regulated cloud-scale star formation efficiency in a simulated dwarf galaxy merger
por: Deng, Yunwei, et al.
Publicado: (2025)

Tracing the cosmological origin of gas that fuels in situ star formation in TNG50 galaxies
por: Wittig, Ole, et al.
Publicado: (2025)

Radiation magnetohydrodynamics simulations of Population III star formation during the Epoch of Reionization
por: van Veenen, Lisanne, et al.
Publicado: (2025)

Massive black hole formation in Population III star clusters
por: Reinoso, B., et al.
Publicado: (2025)

SIEGE IV: compact star clusters in cosmological simulations with high star formation efficiency and sub-parsec resolution
por: Pascale, R., et al.
Publicado: (2025)

DRAGON-III simulation: modelling million-body globular and nuclear star clusters
por: Wu, Kai, et al.
Publicado: (2025)

A subgrid model for chemical enrichment in cosmological simulations
por: Correa, Camila A., et al.
Publicado: (2026)

Direct N-body simulations of rotating and extremely massive Population III star clusters
por: Wu, Kai, et al.
Publicado: (2026)

On the origin of outward migration of Population III stars
por: Park, Jongwon, et al.
Publicado: (2023)

Zooming in on the circumgalactic medium with GIBLE: Cloud-scale simulations with cosmological initial conditions
por: Ramesh, Rahul, et al.
Publicado: (2026)

Towards a universal analytical model for Population III star formation: interplay between feedback and fragmentation
por: Liu, Boyuan, et al.
Publicado: (2024)

The detection and characterization of highly magnified stars with JWST: Prospects of finding Population III
por: Zackrisson, Erik, et al.
Publicado: (2023)

Population III star formation near high-redshift active galactic nuclei
por: Fisk, Ethan M., et al.
Publicado: (2025)

Hydrodynamic methods and sub-resolution models for cosmological simulations
por: Valentini, Milena, et al.
Publicado: (2025)

On the origin of star formation quenching in massive galaxies at $z \gtrsim 3$ in the cosmological simulations IllustrisTNG
por: Kurinchi-Vendhan, Shalini, et al.
Publicado: (2023)

Local positive feedback in the overall negative: the impact of quasar winds on star formation in the FIRE cosmological simulations
por: Mercedes-Feliz, Jonathan, et al.
Publicado: (2023)

A cosmological framework for stellar collisions at high redshift in proto-globular clusters, nuclear star clusters, and Little Red Dots
por: Williams, Claire E., et al.
Publicado: (2026)

The MAGPI Survey: radial trends in star formation across different cosmological simulations in comparison with observations at $z \sim$ 0.3
por: Mun, Marcie, et al.
Publicado: (2024)

Modeling submillimeter galaxies in cosmological simulations: Contribution to the cosmic star formation density and predictions for future surveys
por: Kumar, Ankit, et al.
Publicado: (2025)

The mass distribution of the first stars can be determined via the 21-cm signal
por: Gessey-Jones, T., et al.
Publicado: (2025)

ArkenstoneBH. A model for high-specific energy black hole feedback in cosmological simulations
por: Sullivan, James M., et al.
Publicado: (2026)

On the rapid growth of SMBHs in high-z galaxies: the aftermath of Population III.1 stars
por: Sanati, Mahsa, et al.
Publicado: (2025)

MEGATRON: The environments of Population III stars at Cosmic Dawn and their connection to present day galaxies
por: Storck, Anatole, et al.
Publicado: (2025)

Introducing the BRAHMA simulation suite: Signatures of low mass black hole seeding models in cosmological simulations
por: Bhowmick, Aklant K., et al.
Publicado: (2024)

The nature of diffuse ionised gas in star-forming galaxies
por: McClymont, William, et al.
Publicado: (2024)

NEATH III: a molecular line survey of a simulated star-forming cloud
por: Priestley, F. D., et al.
Publicado: (2024)

RIGEL: Simulating dwarf galaxies at solar mass resolution with radiative transfer and feedback from individual massive stars
por: Deng, Yunwei, et al.
Publicado: (2024)

Arkenstone -- II. A model for unresolved cool clouds entrained in galactic winds in cosmological simulations
por: Smith, Matthew C., et al.
Publicado: (2024)

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

Testing Jeans dynamical models with prolate rotation on a cosmologically simulated dwarf galaxy
por: Sedain, Amrit, et al.
Publicado: (2023)

MISTRAL: a model for AGN winds from radiatively efficient accretion in cosmological simulations
por: Farcy, Marion, et al.
Publicado: (2025)

The baryon cycle in modern cosmological hydrodynamical simulations
por: Wright, Ruby J., et al.
Publicado: (2024)