Spiral galaxies with flat radial abundance gradients at large radii
Fuente:
arXiv
Guardado en:
| Autores principales: | Pilyugin, L. S., Tautvaisiene, G. |
|---|---|
| Formato: | Preprint |
| Publicado: |
2026
|
| Materias: | |
| Acceso en línea: | |
| Etiquetas: |
Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
|
Ejemplares similares
Spiral galaxies with unusual azimuthal asymmetry in oxygen abundance
por: Pilyugin, L. S., et al.
Publicado: (2025)
por: Pilyugin, L. S., et al.
Publicado: (2025)
Two sequences of spiral galaxies with different shapes of the metallicity gradients
por: Pilyugin, L. S., et al.
Publicado: (2023)
por: Pilyugin, L. S., et al.
Publicado: (2023)
Central oxygen abundances in the spiral galaxies of the MaNGA survey: Galaxies with central starbursts
por: Pilyugin, L. S., et al.
Publicado: (2024)
por: Pilyugin, L. S., et al.
Publicado: (2024)
Temperature based radial metallicity gradients in nearby galaxies
por: Kreckel, K., et al.
Publicado: (2025)
por: Kreckel, K., et al.
Publicado: (2025)
Metal-THINGS: The Milky Way twin candidate NGC 3521
por: Pilyugin, L. S., et al.
Publicado: (2025)
por: Pilyugin, L. S., et al.
Publicado: (2025)
Metal-THINGS: gas metallicity gradients in nearby galaxies
por: Valé, Guillermo, et al.
Publicado: (2025)
por: Valé, Guillermo, et al.
Publicado: (2025)
Puzzling radial gradients of K-band absorption features in the giant elliptical galaxy M87
por: La Barbera, F., et al.
Publicado: (2025)
por: La Barbera, F., et al.
Publicado: (2025)
The abundance and radial distribution of faint and ultra-faint dwarfs in galaxy clusters
por: Sadhu, Pradyumna, et al.
Publicado: (2026)
por: Sadhu, Pradyumna, et al.
Publicado: (2026)
Cross-method analysis of co-rotation radii dataset for spiral galaxies
por: Kostiuk, Valeria S., et al.
Publicado: (2024)
por: Kostiuk, Valeria S., et al.
Publicado: (2024)
The Galactic inner spiral arms revealed by the Gaia ESO Survey chemical abundances. Metallicity and [Mg/Fe] ratios
por: Vázquez, C. Viscasillas, et al.
Publicado: (2025)
por: Vázquez, C. Viscasillas, et al.
Publicado: (2025)
The physical origin of positive metallicity radial gradients in high-redshift galaxies: insights from the FIRE-2 cosmological hydrodynamic simulations
por: Sun, Xunda, et al.
Publicado: (2024)
por: Sun, Xunda, et al.
Publicado: (2024)
CO radial gradients in the bulge of M31
por: La Barbera, F., et al.
Publicado: (2024)
por: La Barbera, F., et al.
Publicado: (2024)
Influence of star cluster mass, age, and galaxy star formation rate on star cluster radii
por: Sebastian, Michelle
Publicado: (2026)
por: Sebastian, Michelle
Publicado: (2026)
The S-PLUS Fornax Project (S+FP): An extragalactic catalog covering $\sim$ 5 virial radii around NGC 1399 with galaxy properties
por: Haack, R. F., et al.
Publicado: (2026)
por: Haack, R. F., et al.
Publicado: (2026)
The Three Hundred Project: The relationship between the shock and splashback radii of simulated galaxy clusters
por: Zhang, M., et al.
Publicado: (2024)
por: Zhang, M., et al.
Publicado: (2024)
New radial velocities for 40 nearby dwarf galaxies
por: Karachentsev, Igor D., et al.
Publicado: (2024)
por: Karachentsev, Igor D., et al.
Publicado: (2024)
Chemical abundances of LINER galaxies -- Nitrogen abundance estimations
por: Oliveira Jr., C. B., et al.
Publicado: (2024)
por: Oliveira Jr., C. B., et al.
Publicado: (2024)
Boundary-supported radial layering in Hoag-like ring galaxies
por: Xu, Yue, et al.
Publicado: (2026)
por: Xu, Yue, et al.
Publicado: (2026)
A strong falsification of the universal radial acceleration relation in galaxies
por: Chan, Man Ho
Publicado: (2024)
por: Chan, Man Ho
Publicado: (2024)
Breaking the degeneracy between warps and radial flows in external galaxies
por: Labini, Francesco Sylos, et al.
Publicado: (2025)
por: Labini, Francesco Sylos, et al.
Publicado: (2025)
Consequences of radially correlated rotation curves for galaxy mass models
por: Chase, Helena, et al.
Publicado: (2025)
por: Chase, Helena, et al.
Publicado: (2025)
Mapping radial abundance gradients with Gaia-ESO open clusters: Evidence of recent gas accretion in the Milky Way disk
por: Palla, Marco, et al.
Publicado: (2024)
por: Palla, Marco, et al.
Publicado: (2024)
Distinct radial acceleration relations of galaxies and galaxy clusters supports hyperconical modified gravity
por: Monjo, Robert, et al.
Publicado: (2024)
por: Monjo, Robert, et al.
Publicado: (2024)
Shape asymmetries and the relation between lopsidedness and radial alignment in simulated galaxies
por: Shen, Jinzhi, et al.
Publicado: (2022)
por: Shen, Jinzhi, et al.
Publicado: (2022)
Why do galaxies have extended flat rotation curves?
por: Hoeneisen, Bruce
Publicado: (2024)
por: Hoeneisen, Bruce
Publicado: (2024)
Gas-phase metallicity gradients in galaxies at $z \sim 6-8$
por: Venturi, G., et al.
Publicado: (2024)
por: Venturi, G., et al.
Publicado: (2024)
GALAXY CRUISE: Spiral and ring classifications for bright galaxies at z=0.01-0.3
por: Shimakawa, Rhythm, et al.
Publicado: (2023)
por: Shimakawa, Rhythm, et al.
Publicado: (2023)
The radial orbits of ram-pressure-stripped galaxies in clusters from the GASP survey
por: Biviano, A., et al.
Publicado: (2024)
por: Biviano, A., et al.
Publicado: (2024)
Chemical radial gradients for the bulge-bar stellar populations from the APOGEE survey
por: Sales-Silva, J. V., et al.
Publicado: (2026)
por: Sales-Silva, J. V., et al.
Publicado: (2026)
On the fundamentality of the radial acceleration relation for late-type galaxy dynamics
por: Stiskalek, Richard, et al.
Publicado: (2023)
por: Stiskalek, Richard, et al.
Publicado: (2023)
The Gaia-ESO Survey: No sign of multiple stellar populations in open clusters from their sodium and oxygen abundances
por: Bragaglia, A., et al.
Publicado: (2024)
por: Bragaglia, A., et al.
Publicado: (2024)
Testable predictions of outside-in age gradients in dwarf galaxies of all types
por: Riggs, Claire L., et al.
Publicado: (2024)
por: Riggs, Claire L., et al.
Publicado: (2024)
The ALPINE-CRISTAL-JWST Survey: Gas-phase abundance gradients of main sequence star-forming galaxies and their kinematics at $4 < z < 6$
por: Lee, Lilian L., et al.
Publicado: (2026)
por: Lee, Lilian L., et al.
Publicado: (2026)
Parallax-based Distances to Galactic Hii Regions: Nearby Spiral Structure
por: Shen, X. J., et al.
Publicado: (2025)
por: Shen, X. J., et al.
Publicado: (2025)
The radial acceleration relation at the EDGE of galaxy formation: testing its universality in low-mass dwarf galaxies
por: Júlio, Mariana P., et al.
Publicado: (2025)
por: Júlio, Mariana P., et al.
Publicado: (2025)
Living with Neighbors. V. Better-aligned Spiral+Spiral Galaxy Pairs Show Stronger Star Formation
por: Zee, Woong-Bae G., et al.
Publicado: (2025)
por: Zee, Woong-Bae G., 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)
por: Scalco, Michele, et al.
Publicado: (2024)
The splashback radius and the radial velocity profile of galaxy clusters in IllustrisTNG
por: Pizzardo, Michele, et al.
Publicado: (2023)
por: Pizzardo, Michele, et al.
Publicado: (2023)
Chemical enrichment in LINERs from MaNGA. II. Characterizing the shape of their radial metallicity gradients
por: Pérez-Díaz, Borja, et al.
Publicado: (2025)
por: Pérez-Díaz, Borja, et al.
Publicado: (2025)
Evolution of the radial ISM metallicity gradient in the Milky Way disk since redshift $\approx 3$
por: Ratcliffe, Bridget, et al.
Publicado: (2024)
por: Ratcliffe, Bridget, et al.
Publicado: (2024)
Ejemplares similares
-
Spiral galaxies with unusual azimuthal asymmetry in oxygen abundance
por: Pilyugin, L. S., et al.
Publicado: (2025) -
Two sequences of spiral galaxies with different shapes of the metallicity gradients
por: Pilyugin, L. S., et al.
Publicado: (2023) -
Central oxygen abundances in the spiral galaxies of the MaNGA survey: Galaxies with central starbursts
por: Pilyugin, L. S., et al.
Publicado: (2024) -
Temperature based radial metallicity gradients in nearby galaxies
por: Kreckel, K., et al.
Publicado: (2025) -
Metal-THINGS: The Milky Way twin candidate NGC 3521
por: Pilyugin, L. S., et al.
Publicado: (2025)