Results 11 to 20 of about 52,268 (222)

He abundances in disc galaxies. I. Predictions from cosmological chemodynamical simulations [PDF]

open access: yesAstronomy & Astrophysics, 2019
Accepted for publication in A&AWe investigate how the stellar and gas-phase He abundances evolve as a function of time within simulated star-forming disc galaxies with different star formation histories.
Kobayashi, Chiaki   +4 more
core   +7 more sources

Dust Formation in a Galaxy with Primitive Abundances [PDF]

open access: yesScience, 2009
Interstellar dust plays a crucial role in the evolution of galaxies. It governs the chemistry and physics of the interstellar medium. In the local universe, dust forms primarily in the ejecta from stars, but its composition and origin in galaxies at very early times remain controversial.
Sloan, G C   +8 more
openaire   +6 more sources

Chemical abundances in Seyfert galaxies – VIII. Argon abundance estimates [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2021
ABSTRACT For the first time, the argon abundance relative to hydrogen abundance (Ar/H) in the narrow line region of a sample of Seyfert 2 nuclei has been derived. In view of this, optical narrow emission line intensities of a sample of 64 local Seyfert 2 nuclei (z < 0.25) taken from Sloan Digital Sky Survey DR7 and measured by the
A F Monteiro, O L Dors
  +7 more sources

Chemical abundances in active galaxies [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2020
ABSTRACT The Sloan Digital Sky Survey (SDSS) has proved to be a powerful resource for understanding the physical properties and chemical composition of star-forming galaxies in the local Universe. The SDSS population of active galactic nuclei (AGNs) remains as of yet less explored in this capacity.
Flury, Sophia R., Moran, Edward C.
openaire   +2 more sources

Abundance of field galaxies [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2015
15 pages, 13 figures.
Klypin, Anatoly   +3 more
openaire   +2 more sources

Abundance ratios in dwarf elliptical galaxies [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2017
We determine abundance ratios of 37 dwarf ellipticals (dEs) in the nearby Virgo cluster. This sample is representative of the early-type population of galaxies in the absolute magnitude range -19.0 < Mr < -16.0. We analyze their absorption line-strength indices by means of index-index diagrams and scaling relations and use the stellar population ...
Şen, Ş.   +16 more
openaire   +9 more sources

Abundance Ratios in Dwarf Elliptical Galaxies [PDF]

open access: yesProceedings of the International Astronomical Union, 2016
AbstractThe aim of this study is to determine abundance ratios and star formation histories (SFH) of dwarf ellipticals in the nearby Virgo cluster. We perform a stellar population analysis of 39 dEs and study them using index-index and scaling relations. We find an unusual behaviour where [Na/Fe] is under-abundant w.r.t.
Sen, Seyda   +3 more
openaire   +4 more sources

Chemical abundances in Seyfert galaxies – X. Sulphur abundance estimates

open access: yesMonthly Notices of the Royal Astronomical Society, 2023
ABSTRACT For the first time, the sulphur abundance relative to hydrogen (S/H) in the narrow-line regions of a sample of Seyfert 2 nuclei (Sy 2s) has been derived via direct estimation of the electron temperature. Narrow emission-line intensities from the Sloan Digital Sky Survey (SDSS) Data Release 17 (DR17) [in the wavelength range 3000
Oli L Dors   +14 more
openaire   +3 more sources

Modeling abundances in galaxies [PDF]

open access: yesProceedings of the International Astronomical Union, 2015
AbstractWe reviewed chemical evolution of galaxies using our cosmological simulations.
Chiaki Kobayashi, Philip Taylor
openaire   +1 more source

Stellar Abundances in Local Group Galaxies [PDF]

open access: yesHighlights of Astronomy, 2005
AbstractHere we describe some of our latest results from measuring detailed abundances in Local Group dwarf galaxies with the VLT. Combining spectroscopic abundances with Color-Magnitude diagrams allows the effective measurement of detailed chemical evolution with time in these galaxies.
Tolstoy, Eline, Venn, Kim
openaire   +2 more sources

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