Results 141 to 150 of about 271,788 (231)
Chemical abundances and small-scale gas kinematics in the local star-forming galaxy NGC 2366
International audienceWe present a detailed spectroscopic study of ionised gas in the nearby (~3.3Mpc) dwarf galaxy NGC 2366, a local analogue of Green Pea galaxies, based on observations with the SCORPIO-2 instrument at the Russian 6-m BTA telescope ...
Moiseev, Alexei V +5 more
core +1 more source
APOGEE Chemical Abundances of the Sagittarius Dwarf Galaxy
Indexación: ScopusThe Apache Point Observatory Galactic Evolution Experiment provides the opportunity of measuring elemental abundances for C, N, O, Na, Mg, Al, Si, P, K, Ca, V, Cr, Mn, Fe, Co, and Ni in vast numbers of stars.
Verne Smith +54 more
core +1 more source
Iron Snails: Nonequilibrium Dynamics and Spiral Abundance Patterns
Galaxies are not in a dynamical steady state: they continually undergo perturbations, e.g., from infalling dwarf galaxies and dark matter substructure. After a dynamical perturbation, stars phase mix toward a new steady state; in so doing, they generally
Neige Frankel +4 more
doaj +1 more source
Chemical Abundance Gradients in Open Clusters from the Gaia/LAMOST Sample
Based on a large and homogeneous sample of 299 open clusters (OCs) from Gaia DR3 and large sky area multiobject fiber spectroscopic telescope DR11, we studied the abundance gradients of the α -elements Mg and Si, and the iron-peak elements Fe and Ni to ...
Guochao Yang +5 more
doaj +1 more source
In addition to comprehensive surveys of the Milky Way (MW) bulge, disk, and halo, the Apache Point Galactic Evolution Experiment (APOGEE) project observed seven dwarf spheroidal satellites (dSphs) of the MW: Carina, Sextans, Sculptor, Draco, Ursa Minor ...
Matthew Shetrone +12 more
doaj +1 more source
The Hot and Energetic Universe:The evolution of galaxy groups and clusters [PDF]
Major astrophysical questions related to the formation and evolution of structures, and more specifically of galaxy groups and clusters, will still be open in the coming decade and beyond: what is the interplay of galaxy, supermassive black hole, and ...
Bourdin, H. +47 more
core
The High-Redshift Gas-Phase Mass–Metallicity Relation in FIRE-2
The unprecedented infrared spectroscopic capabilities of JWST have provided high-quality interstellar medium metallicity measurements and enabled characterization of the gas-phase mass–metallicity relation (MZR) for galaxies at z ≳ 5 for the first time ...
Andrew Marszewski +4 more
doaj +1 more source
This study probes the chemical abundances of the neutron-capture elements cerium and neodymium in the inner Milky Way from an analysis of a sample of ∼2000 stars in the Galactic bulge bar spatially contained within ∣ X _Gal ∣ < 5 kpc, ∣ Y _Gal ∣ < 3.5 ...
J. V. Sales-Silva +30 more
doaj +1 more source
Accurate determination of chemical abundances near a supermassive black hole. [PDF]
XRISM Collaboration.
europepmc +1 more source
Galactic outflows and star-formation quenching: a JWST perspective. [PDF]
Davies RL, Belli S.
europepmc +1 more source

