Chemical abundance patterns in Local Group galaxies within cosmological simulations

In the context of the concordance cosmology, structure formation in the universe is the result of the amplification, by gravitational effects, of small perturbations in the primeval density field. This results in the formation of structures known as dark matter haloes, where gas collapses and forms...

Descripción completa

Guardado en:

Detalles Bibliográficos
Autores principales:	Biaus, L., Scannapieco, C., Nuza, S. E.
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2021
Materias:	Ciencias Astronómicas galaxies: structure galaxies: abundances methods: numerical
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/168929
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

Ejemplares similares

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

Cosmological simulations of the formation and evolution of Milky Way-mass galaxies
por: Scannapieco, Cecilia
Publicado: (2023)

The evolution of galaxy metallicity scaling relations in cosmological hydrodynamical simulations
por: De Rossi, M.E., et al.

The evolution of galaxy metallicity scaling relations in cosmological hydrodynamical simulations
Publicado: (2015)

Kinematics of the Local Group gas and galaxies in the Hestia simulations
por: Biaus, Luis, et al.
Publicado: (2023)

Chemical evolution using smooth particle hydrodynamical cosmological simulations - I. Implementation, tests and first results
por: Mosconi, M. B., et al.
Publicado: (2001)

Insight into the physical processes that shape the metallicity profiles in galaxies
por: Tapia, B., et al.
Publicado: (2022)

Galaxy pairs in cosmological simulations: Effects of interactions on colours and chemical abundances
por: Perez, María Josefa, et al.
Publicado: (2006)

Galaxy pairs in cosmological simulations: Effects of interactions on star formation
por: Perez, María Josefa, et al.
Publicado: (2006)

Gas accretion onto the disc of a simulated Milky Way-mass galaxy
por: Iza, F. G., et al.
Publicado: (2021)

Local metallicity in simulated galaxies
por: Collacchioni, Florencia, et al.
Publicado: (2021)

The temporal evolution of gas accretion onto the discs of simulated Milky Way-mass galaxies
por: Iza, Federico, et al.
Publicado: (2023)

Feedback and metal enrichment in cosmological smoothed particle hydrodynamics simulations - I. A model for chemical enrichment
por: Scannapieco, C., et al.

Simulations of MW-mass galaxies in the cosmological context
por: Scannapieco, C.

Age and metallicity gradients in simulated galaxies of the Local Group
por: Marioni, O. F., et al.
Publicado: (2021)

Linking gaseous and stellar gradients on simulated galaxies of the Local Group
por: Marioni, Ornela, et al.
Publicado: (2023)

Feedback and metal enrichment in cosmological smoothed particle hydrodynamics simulations - I. A model for chemical enrichment
Publicado: (2005)

Connection between feedback processes and the effective yields of EAGLE galaxies
por: Zerbo, María Candela, et al.
Publicado: (2024)

Chemical abundance of the LINER galaxy UGC 4805 with SDSS-IV MaNGA
por: Krabbe, Angela, et al.
Publicado: (2021)

Chemical evolution using smooth particle hydrodynamical cosmological simulations - I. Implementation, tests and first results
por: Mosconi, M.B., et al.

Chemical evolution using smooth particle hydrodynamical cosmological simulations - I. Implementation, tests and first results
Publicado: (2001)

Effects of feedback processes on the effective yields of galaxies
por: Zerbo, María Candela, et al.
Publicado: (2022)

Galaxy pairs in cosmological simulations: Effects of interactions on colours and chemical abundances
por: Perez, M.J., et al.

Chemical abundances in Seyfert galaxies – V. The discovery of shocked emission outside the AGN ionization axis
por: Riffel, R. A., et al.
Publicado: (2020)

Effective yields as tracers of feedback effects on the metal enrichment of galaxies
por: Zerbo, María Candela, et al.
Publicado: (2023)

Effects of supernova feedback on the formation of galaxy discs
por: Scannapieco, C., et al.

Simulations of MW-mass galaxies in the cosmological context
Publicado: (2017)

Connection between the star formation activity and stellar metallicities of galaxies in cosmological simulations
por: Grimozzi, Salvador, et al.
Publicado: (2022)

Galaxy pairs in cosmological simulations: Effects of interactions on colours and chemical abundances
Publicado: (2006)

The effect of gas accretion on the radial gas metallicity profile of simulated galaxies
por: Collacchioni, Florencia, et al.
Publicado: (2020)

Chemoarchaeological downsizing in a hierarchical universe: impact of a top-heavy IGIMF
por: Gargiulo, Ignacio Daniel, et al.
Publicado: (2014)

Chemical abundances of Seyfert 2 AGNs - I. Comparing oxygen abundances from distinct methods using SDSS
por: Dors, O. L., et al.
Publicado: (2019)

TYPE Ia SUPERNOVA PROGENITORS and CHEMICAL ENRICHMENT in HYDRODYNAMICAL SIMULATIONS. I. the SINGLE-DEGENERATE SCENARIO
por: Jiménez, N., et al.

TYPE Ia SUPERNOVA PROGENITORS and CHEMICAL ENRICHMENT in HYDRODYNAMICAL SIMULATIONS. I. the SINGLE-DEGENERATE SCENARIO
Publicado: (2015)

Chemical properties of galaxy baryons as a function of halo mass in a ΛCDM cosmology
por: Burrafato, Y. D., et al.
Publicado: (2024)

Effects of supernova feedback on the formation of galaxy discs
Publicado: (2008)

Chemical evolution during gas-rich galaxy interactions
por: Perez, María Josefa, et al.
Publicado: (2011)

Chemical abundances of Seyfert 2 AGNs – III. Reducing the oxygen abundance discrepancy
por: Dors, Oli L., et al.
Publicado: (2020)

Chemical abundances in Seyfert galaxies – VII. Direct abundance determination of neon based on optical and infrared emission lines
por: Armah, Mark, et al.
Publicado: (2021)

Extragalactic Star-forming Regions: a Study of the Physical Properties and Chemical Abundances
por: Muñoz-Vergara, Dania, et al.
Publicado: (2019)