Results 181 to 190 of about 948,048 (332)
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
Oxygen Abundances in the Milky Way Using X‐Ray Absorption Measurements toward Galaxy Clusters [PDF]
W. H. Baumgartner, R. F. Mushotzky
openalex +1 more source
The variation of carbon abundance in galaxies and its implications [PDF]
D. Romano +5 more
openalex +1 more source
Zingiber odoriferum (Zingiberaceae), a critically endangered ginger species endemic to Java, Indonesia, is ecologically vital yet genomically understudied. We present the first complete chloroplast (cp) genome (163 538 bp), revealing a quadripartite structure with a large single‐copy region (88 033 bp), a small single‐copy region (15 885 bp), and a ...
Irfan Martiansyah +5 more
wiley +1 more source
Weak-Lensing Shear-Selected Galaxy Clusters from the Hyper Suprime-Cam Subaru Strategic Program: II. Cosmological Constraints from the Cluster Abundance [PDF]
I. Chiu +10 more
openalex +2 more sources
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
Predictions for complex distributions of stellar elemental abundances in low-mass galaxies [PDF]
P. Patel +5 more
openalex +1 more source
Oxychlorine Species on Mars: A Review
Abstract Oxychlorine species (mainly perchlorate and chlorate) have been identified at multiple locations on the surface of Mars by both orbiter and in situ rovers. They have also been found in martian meteorites. Cl‐isotopes in meteoritic minerals suggest that an oxychlorine cycle has been operating on the martian surface for the last ∼4 billion years.
Kaushik Mitra
wiley +1 more source
XMM Observations of Metal Abundances in Galaxy Clusters
The hot gas that fills the space between galaxies in clusters is rich in metals. Due to their large potential well, galaxy clusters accumulate metals over the whole history of the cluster, and retain important information on cluster formation and ...
L. Lovisari, S. Schindler, W. Kapferer
doaj
We describe new ultradeep James Webb Space Telescope (JWST) NIRSpec PRISM and grating spectra for the galaxies JADES-GS-z11-0 ( ${z}_{\mathrm{spec}}={11.122}_{-0.003}^{+0.005}$ ) and JADES-GS-z13-0 ( ${z}_{\mathrm{spec}}={13.20}_{-0.04}^{+0.03}$ ), the ...
Kevin N. Hainline +31 more
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