Imagen de Portada

Phase-space mixing of multiple stellar populations in globular clusters

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Aros, Francisco I., Vesperini, Enrico, Dalessandro, Emanuele
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

The structural properties of multiple populations in globular clusters: the instructive case of NGC 3201
por: Cadelano, Mario, et al.
Publicado: (2024)

Evolution of the kinematic properties of rotating multiple-population globular clusters
por: White, Ethan B., et al.
Publicado: (2025)

Energy equipartition in multiple-population globular clusters
por: Livernois, A. R., et al.
Publicado: (2024)

A 3D view of multiple populations kinematics in Galactic globular clusters
por: Dalessandro, E., et al.
Publicado: (2024)

MOCCA: Global properties of tidally filling and underfilling globular star clusters with multiple stellar populations
por: Hypki, Arkadiusz, et al.
Publicado: (2024)

Structural parameters, chronological age and dynamical age of the LMC globular cluster NGC 1754
por: Giusti, Camilla, et al.
Publicado: (2025)

Inference of black-hole mass fraction in Galactic globular clusters. A multi-dimensional approach to break the initial-condition degeneracies
por: Della Croce, A., et al.
Publicado: (2024)

The dynamical age of the LMC globular cluster NGC 1835 using the "dynamical clock"
por: Giusti, Camilla, et al.
Publicado: (2024)

Revealing the stellar population of the ultra-obscured Galactic globular cluster Glimpse-C02
por: Loriga, M., et al.
Publicado: (2026)

Discovery of an extended Horizontal Branch in the Large Magellanic Cloud globular cluster NGC1835
por: Giusti, Camilla, et al.
Publicado: (2024)

Exploring the dynamical evolution of binary stars in multiple-population globular clusters
por: Bruce, J., et al.
Publicado: (2026)

Insights into spatial mixing of multiple populations in dynamically-young globular clusters
por: Pavlík, Václav, et al.
Publicado: (2025)

Spatial mixing of stellar populations in globular clusters via binary-single star scattering
por: Pavlík, Václav, et al.
Publicado: (2025)

The HST Large Programme on omega Centauri -- VI. The radial gradient of the stellar populations
por: Scalco, Michele, et al.
Publicado: (2024)

New Parameters for Star Cluster Dynamics: the role of clusters initial conditions
por: Bhat, Bhavana, et al.
Publicado: (2024)

Identification and characterization of optical companions to the population of millisecond pulsars in the globular cluster M3
por: Ettorre, Greta, et al.
Publicado: (2025)

Discrepancies between spectroscopy and HST photometry in tagging multiple stellar populations in 22 globular clusters
por: Carretta, Eugenio, et al.
Publicado: (2024)

A Photometric in-depth look at the core-collapsed globular cluster NGC 6284
por: Deras, Dan, et al.
Publicado: (2023)

MOCCA: Effects of pristine gas accretion and cluster migration on globular cluster evolution, global parameters, and multiple stellar populations
por: Giersz, Mirek, et al.
Publicado: (2024)

Multiple stellar population mass loss in massive Galactic globular clusters
por: Lacchin, Elena, et al.
Publicado: (2023)

Synthetic stellar spectra to study multiple populations in globular clusters: an extended grid and the effects on the integrated light
por: Branco, Vinicius, et al.
Publicado: (2024)

Spectrophotometry in the integrated light of multiple populations in globular clusters
por: Branco, Vinicius, et al.
Publicado: (2025)

Two stellar populations with different metallicities in the low-mass globular cluster Gran 5
por: Lim, Dongwook, et al.
Publicado: (2024)

Linking Photometry and spectroscopy: profiling multiple populations in globular clusters
por: Dondoglio, E., et al.
Publicado: (2025)

Chemo-dynamical reconstruction of Milky Way globular cluster progenitors: Age-metallicity relations and the universality of multiple stellar populations
por: Lardo, Carmela, et al.
Publicado: (2026)

New parameters for star cluster dynamics: observational results
por: Lanzoni, Barbara, et al.
Publicado: (2026)

CAPOS: The bulge Cluster APOGEE Survey VI. Characterizing multiple stellar populations and chemical abundances in the bulge globular cluster NGC 6569
por: Barrera, Nicolás, et al.
Publicado: (2025)

A stellar census in globular clusters with MUSE. Metallicity spread and dispersion among first-population stars
por: Latour, M., et al.
Publicado: (2025)

The bulge globular cluster Terzan 6 as seen from multi-conjugate adaptive optics and HST
por: Loriga, Martina, et al.
Publicado: (2025)

The multi-age stellar populations of Terzan 5 as revealed by JWST
por: Zullo, G., et al.
Publicado: (2026)

Right round: onset and long-term evolution of rotation in star clusters
por: Dalessandro, E., et al.
Publicado: (2026)

Probing populations of dark stellar remnants in the globular clusters 47 Tuc and Terzan 5 using pulsar timing
por: Smith, Peter J., et al.
Publicado: (2024)

The emergence of globular clusters and globular-cluster-like dwarfs
por: Taylor, Ethan D., et al.
Publicado: (2025)

Tracing the W3/W4/W5 and Perseus complex dynamical evolution with star clusters
por: Della Croce, A., et al.
Publicado: (2025)

Gaps in stellar streams as a result of globular cluster fly-bys
por: Ferrone, Salvatore, et al.
Publicado: (2025)

Dynamics of star clusters with tangentially anisotropic velocity distribution
por: Pavlík, Václav, et al.
Publicado: (2024)

An analytical approach to binary populations in globular clusters
por: O'Connor, Christopher E., et al.
Publicado: (2026)

Multiple stellar populations at less evolved stages. IV. evidence of helium enrichments in four Magellanic globular clusters
por: Li, Chengyuan, et al.
Publicado: (2025)

Noble gases Neon and argon: a role for the chemical patterns of multiple populations in globular clusters?
por: Ventura, P., et al.
Publicado: (2026)

Detailed chemical abundances of the globular cluster Terzan 6 in the inner bulge
por: Fanelli, C., et al.
Publicado: (2024)