Imagen de Portada

KRIOS: A new basis-expansion $N$-body code for collisional stellar dynamics

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Tep, Kerwann, Cook, Brian T., Rodriguez, Carl L., Jolly, Jiya, Sawin, Eddie, Petersen, Michael S., Gaffud, Christoph
Formato:	Preprint
Publicado:	2025
Materias:	Astrophysics of Galaxies
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

Linear response of rotating and flattened stellar clusters: the oblate Kuzmin-Kutuzov Stäckel family
por: Tep, Kerwann, et al.
Publicado: (2024)

Modeling Globular Cluster Stellar Streams with a Basis-Expansion N-body Code
por: Cook, Brian T., et al.
Publicado: (2026)

Non-resonant relaxation of rotating globular clusters
por: Tep, Kerwann, et al.
Publicado: (2024)

Very long-term relaxation of harmonic 1D self-gravitating systems
por: Tep, Kerwann, et al.
Publicado: (2026)

EXP: a Python/C++ package for basis function expansion methods in galactic dynamics
por: Petersen, Michael S., et al.
Publicado: (2025)

Formation of collisional ring galaxies in Milgromian dynamics
por: Ma, Li, et al.
Publicado: (2024)

NbodyCP:A direct N-body simulation code for composite stellar populations of single and binary star clusters
por: Li, Zhongmu, et al.
Publicado: (2025)

A comparison of the turbulent dynamo in weakly-collisional and collisional plasmas: from subsonic to supersonic turbulence
por: Chirakkara, Radhika Achikanath, et al.
Publicado: (2025)

Differentiable N-body code for Galactic Dynamics -- Odisseo
por: Viterbo, Giuseppe, et al.
Publicado: (2025)

KRATOS: A large suite of N-body simulations to interpret the stellar kinematics of LMC-like discs
por: Jiménez-Arranz, Ó., et al.
Publicado: (2024)

The radial variation of the LMC-induced reflex motion of the Milky Way disc observed in the stellar halo
por: Yaaqib, Rashid, et al.
Publicado: (2024)

The dynamical evolution of the stellar clumps in the Sparkler galaxy
por: Giunchi, Eric, et al.
Publicado: (2025)

The identification of new Herbig Ae/Be stars from LAMOST DR7
por: Liu, Jialin, et al.
Publicado: (2026)

Testing MOND using the dynamics of nearby stellar streams
por: Koop, Orlin, et al.
Publicado: (2024)

Massive star clusters and clumps in the collisional ring galaxy Arp 147
por: Randriamanakoto, Z., et al.
Publicado: (2026)

A calibrated model for N-body dynamical friction acting on supermassive black holes
por: Genina, Anna, et al.
Publicado: (2024)

Spatially resolved stellar-to-total dynamical mass relation: Radial variations, gradients and profiles of galaxy stellar populations
por: Scholz-Diaz, L., et al.
Publicado: (2026)

Bayesian ages of local young stellar associations I. Through the expansion rate method
por: Olivares, J., et al.
Publicado: (2025)

The S2 orbit and tidally disrupted binaries: indications for collisional depletion in the Galactic center
por: Ashkenazy, Yotam, et al.
Publicado: (2024)

Evidence of radial-migration driven Galactic disc expansion with the U-shape stellar age profile
por: Lian, Jianhui, et al.
Publicado: (2026)

Asymmetry of the tidal tails of open star clusters in direct N-body integrations in Milgrom-law dynamics
por: Pflamm-Altenburg, J.
Publicado: (2024)

Action and energy clustering of stellar streams in deforming Milky Way dark matter haloes
por: Brooks, Richard A. N., et al.
Publicado: (2024)

The internal kinematics of local young stellar associations. Identifying correlations among age, expansion, rotation, and shear
por: Olivares, J., et al.
Publicado: (2026)

Baryonic properties of nearby galaxies across the stellar-to-total dynamical mass relation
por: Scholz-Diaz, Laura, et al.
Publicado: (2024)

Quantifying the stellar ages of dynamically separated bulges and disks of CALIFA spiral galaxies
por: Jin, Yunpeng, et al.
Publicado: (2023)

A stellar dynamical mass measure of an inactive black hole in the distant universe
por: Newman, Andrew B., et al.
Publicado: (2025)

Chemo-dynamics of the stellar component of the Sculptor dwarf galaxy I: observed properties
por: Arroyo-Polonio, José María, et al.
Publicado: (2024)

Chemo-dynamics of the stellar component of the Sculptor dwarf galaxy II: dynamical properties and dark matter halo density
por: Polonio, José María Arroyo, et al.
Publicado: (2025)

Exploring biases in derived stellar parameters and the ionizing photon production efficiency
por: Jaiswar, Ravi, et al.
Publicado: (2026)

Going Bayesian on the ages of nearby young stellar systems I. The expansion rate method
por: Olivares, J., et al.
Publicado: (2025)

Discovery of a kinematically distinct component in the central region of the collisional ring galaxy AM0644-741
por: Mondal, Chayan, et al.
Publicado: (2025)

Beyond compactness: a structural-dynamical-evolutionary manifold for the stellar-to-dynamical mass ratio in ultra-compact massive galaxies
por: Spiniello, Chiara
Publicado: (2026)

Geometry of the Milky Way's dark matter from dynamical models of the tilted stellar halo
por: Dillamore, Adam M., et al.
Publicado: (2025)

Photometric vs dynamical stellar masses and their impact on scaling relations in nearby disc galaxies
por: Marasco, A., et al.
Publicado: (2025)

Impacts of stellar wind and supernovae on the star cluster formation: origins of extremely high N/O ratios and multiple stellar populations
por: Fukushima, Hajime, et al.
Publicado: (2024)

The stellar Fundamental Metallicity Relation: the correlation between stellar mass, star-formation rate and stellar metallicity
por: Looser, Tobias J., et al.
Publicado: (2024)

Auriga Superstars: Improving the resolution and fidelity of stellar dynamics in cosmological galaxy simulations
por: Pakmor, Ruediger, et al.
Publicado: (2025)

Superbubbles as the source of dynamical friction: gas migration, stellar and dark matter contributions
por: Kipper, Rain, et al.
Publicado: (2024)

Calibrating the SIDM Gravothermal Catastrophe with N-body Simulations
por: Mace, Charlie, et al.
Publicado: (2025)

Deuteration of HC3N and CH3CCH in the pre-stellar core L1544
por: Giers, K., et al.
Publicado: (2026)