Results 111 to 120 of about 58,855 (236)

Leonessa: An Extremely Metal-poor Galaxy Undergoing Secular Chemical Evolution

open access: yesThe Astrophysical Journal
Extremely metal-poor (XMP) galaxies are systems with gas-phase oxygen abundances below ∼5% solar metallicity (12+log(O/H) ≤ 7.35). These galaxies populate the metal-poor end of the mass–metallicity and luminosity–metallicity relations (MZR and LZR ...
Joseph A. Breneman   +7 more
doaj   +1 more source

Chemical evolution of irregular galaxies

open access: yes, 1998
10 pages, 3 figs, uses moriond.sty. Review presented at XVIIIth Rencontre de Moriond `Dwarf Galaxies and Cosmology', eds.
openaire   +2 more sources

A North–South Metallicity Asymmetry in the Outer Galactic Disk—Evidence for the Pericentric Passage of the Sagittarius Dwarf Galaxy

open access: yesThe Astrophysical Journal Letters
We present maps of the mean metallicity distributions on the Galactocentric R – Z plane at different azimuthal angles using red clump stars selected from the LAMOST and APOGEE surveys.
Chun Wang   +6 more
doaj   +1 more source

Evidence of Truly Young High-α Dwarf Stars

open access: yesThe Astronomical Journal
The existence of high- α stars with inferred ages
Yuxi(Lucy) Lu   +16 more
doaj   +1 more source

Optical Spectroscopy Reveals Hidden Neutron-capture Elemental Abundance Differences among APOGEE-identified Chemical Doppelgängers

open access: yesThe Astrophysical Journal
Grouping stars by chemical similarity has the potential to reveal the Milky Way’s evolutionary history. The APOGEE stellar spectroscopic survey has the resolution and sensitivity for this task.
Catherine Manea   +11 more
doaj   +1 more source

Dynamical and chemical evolution of gas-rich dwarf galaxies [PDF]

open access: green, 2001
S. Recchi, F. Matteuccí, A. D’Ercole
openalex   +1 more source

Early Chemical Evolution of Galaxies

open access: yes, 1999
Initial conditions are set by Big bang nucleosynthesis from which we know that 90 per cent of baryons are dark and have essentially unknown chemical composition. In our own Galaxy, there are many clues from individual stars in different populations whereas in elliptical galaxies the data largely come from integrated spectra, but these raise problems ...
openaire   +2 more sources

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