Imagen de Portada

Centrally concentrated star formation in young clusters

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Assilkhan, Adilkhan, Mac Low, Mordecai-Mark, Polak, Brooke, Abdikamalov, Ernazar, Cournoyer-Cloutier, Claude, Lewis, Sean C., Kalambay, Mukhagali, Otebay, Aigerim, Shukirgaliyev, Bekdaulet
Formato:	Preprint
Publicado:	2025
Materias:	Astrophysics of Galaxies Solar and Stellar Astrophysics
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

Evolution of fractality in centrally concentrated young clusters
por: Akhmetali, Almat, et al.
Publicado: (2026)

Formation and disruption of wide binaries in star clusters revealed by N-body simulations
por: Bissekenov, Abylay, et al.
Publicado: (2026)

Radiation shielding of protoplanetary discs in young star-forming regions
por: Wilhelm, Maite J. C., et al.
Publicado: (2023)

Massive star cluster formation II. Runaway stars as fossils of sub-cluster mergers
por: Polak, Brooke, et al.
Publicado: (2024)

Massive star cluster formation III. Early mass segregation during cluster assembly
por: Polak, Brooke, et al.
Publicado: (2024)

Probing nuclear physics with supernova gravitational waves and machine learning
por: Mitra, Ayan, et al.
Publicado: (2023)

Massive star cluster formation I. High star formation efficiency while resolving feedback of individual stars
por: Polak, Brooke, et al.
Publicado: (2023)

Transferring Data from a Voronoi Mesh to an Adaptive Cartesian Grid in Pursuit of Self-consistent Top-down Star Formation
por: Lewis, Sean C., et al.
Publicado: (2025)

Evaluating Machine Learning Models for Supernova Gravitational Wave Signal Classification
por: Abylkairov, Y. Sultan, et al.
Publicado: (2024)

Convective vortices in collapsing stars
por: Telman, Yerassyl, et al.
Publicado: (2024)

Early-Forming Massive Stars Suppress Star Formation and Hierarchical Cluster Assembly
por: Lewis, Sean C., et al.
Publicado: (2022)

Cluster membership analysis with supervised learning and $N$-body simulations
por: Bissekenov, A., et al.
Publicado: (2024)

Massive Star Cluster Formation with Binaries. I. Evolution of Binary Populations
por: Cournoyer-Cloutier, Claude, et al.
Publicado: (2024)

Fractal dimension of star clusters
por: Ussipov, N., et al.
Publicado: (2024)

Protostellar Jets in Star Cluster Formation and Evolution: I. Implementation and Initial Results
por: Appel, Sabrina M., et al.
Publicado: (2025)

Massive Interacting Binaries Enhance Feedback in Star-Forming Regions
por: Cournoyer-Cloutier, Claude, et al.
Publicado: (2025)

Early Evolution and 3D Structure of Embedded Star Clusters
por: Cournoyer-Cloutier, Claude, et al.
Publicado: (2023)

Reverse and forward shock afterglow emission from steep jets viewed off axis
por: Abdikamalov, Ernazar, et al.
Publicado: (2025)

Pre-supernova feedback sets the star cluster mass function to a power law and reduces the cluster formation efficiency
por: Andersson, Eric P., et al.
Publicado: (2023)

Conference Summary: Stellar Feedback in the ISM: Celebrating the Life and Work of You-Hua Chu
por: Mac Low, Mordecai-Mark
Publicado: (2024)

Evolution of star clusters with initial bulk rotation via N-body simulations
por: Bissekenov, Abylay, et al.
Publicado: (2025)

Systematic Study of Forward and Reverse Shock Afterglow Emission from Two-Component Jets
por: Mukazhanov, Olzhas, et al.
Publicado: (2026)

The Evolution of Substructure during Star Cluster Assembly
por: Laverde-Villarreal, Edwin, et al.
Publicado: (2025)

Dynamical evolution of the open clusters with different star formation efficiencies and orbital parameters
por: Ishchenko, M., et al.
Publicado: (2025)

Binary Disruption and Ejected Stars from Hierarchical Star Cluster Assembly
por: Cournoyer-Cloutier, Claude, et al.
Publicado: (2024)

Kinematic substructure in star clusters constrains star cluster formation
por: Arnold, Becky, et al.
Publicado: (2024)

STARFORGE: Toward a comprehensive numerical model of star cluster formation and feedback
por: Grudić, Michael Y., et al.
Publicado: (2020)

Stellar Feedback Effects on the Mass Distribution of Clouds and Cloud Complexes
por: Quinalha, Luanna Veroneze, et al.
Publicado: (2025)

The contribution to Galactic Centre γ-ray excess from cluster-born millisecond pulsars. Constraints from direct N-body simulations
por: Kalambay, M., et al.
Publicado: (2026)

Cloud-cloud collision and star formation in G013.313+0.193
por: Berdikhan, Dilda, et al.
Publicado: (2025)

Computational approaches to modeling dynamos in galaxies
por: Korpi-Lagg, Maarit J., et al.
Publicado: (2024)

The Importance of Tidal Forces in Molecular Cloud Dynamics
por: Lee, JinWoo, et al.
Publicado: (2025)

Transition from small-scale to large-scale dynamo in a supernova-driven, multiphase medium
por: Gent, Frederick A., et al.
Publicado: (2023)

Dynamical evolution of Milky Way globular clusters on the cosmological timescale I. Mass loss and interaction with the nuclear star cluster
por: Ishchenko, M., et al.
Publicado: (2024)

Quantifying the scale of star formation across the Perseus spiral arm using young clusters around Cas OB5
por: Quintana, Alexis L., et al.
Publicado: (2025)

Planetesimal formation via the streaming instability persists under turbulence driven by magnetorotational instability
por: Eriksson, Linn E. J., et al.
Publicado: (2026)

The emerging timescale of young star clusters regulated by cluster stellar mass
por: Pedrini, Alex, et al.
Publicado: (2026)

Accretion bursts in young intermediate-mass stars make planet formation challenging
por: Das, Indrani, et al.
Publicado: (2025)

Effects of helium sedimentation on late star formation in galaxy clusters
por: Racker, J., et al.
Publicado: (2025)

Most nearby young star clusters formed in three massive complexes
por: Swiggum, Cameren, et al.
Publicado: (2024)