Results 131 to 140 of about 205,088 (284)

Chemical abundances in spiral and irregular galaxies. O and N abundances derived from global emission--line spectra

open access: yes, 2004
The validity of oxygen and nitrogen abundances derived from the global emission-line spectra of galaxies via the P-method has been investigated using a collection of published spectra of individual HII regions in irregular and spiral galaxies.
Carollo   +31 more
core   +1 more source

Abundances in Virgo spiral galaxies [PDF]

open access: yesPublications of the Astronomical Society of the Pacific, 1991
oxygen abundances substantially higher than in comparable field galaxies. Possible causes include stripping of the outer hydrogen disk and curtailment of cosmological infall in the cluster environment.
openaire   +2 more sources

Technical considerations and review of urinary microRNAs as biomarkers for chronic kidney disease in dogs and cats

open access: yesVeterinary Clinical Pathology, EarlyView.
Abstract MicroRNAs (miRNAs or miRs) are small, non‐coding RNAs that play a crucial role in gene regulation, making them potential biomarkers for various diseases. In the field of veterinary medicine, there is a growing interest in exploring the diagnostic and therapeutic potential of miRNAs in kidney diseases affecting dogs and cats.
Candice P. Chu, Mary B. Nabity
wiley   +1 more source

Chemical Abundance Gradients in Open Clusters from the Gaia/LAMOST Sample

open access: yesThe Astronomical Journal
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

Abundances and gradients in nearby galaxies [PDF]

open access: yesProceedings of the International Astronomical Union, 2016
AbstractThe study of chemical abundance gradients can provide essential information on the evolution of disk galaxies. Here I briefly review our current observational knowledge concerning the abundances of the ionized gas (H ii regions and planetary nebulae) in nearby galaxies, and how they inform us about the time evolution of metallicity gradients.
openaire   +2 more sources

Revolutionizing multi‐omics analysis with artificial intelligence and data processing

open access: yesQuantitative Biology, Volume 13, Issue 3, September 2025.
Abstract Our understanding of intricate biological systems has been completely transformed by the development of multi‐omics approaches, which entail the simultaneous study of several different molecular data types. However, there are many obstacles to overcome when analyzing multi‐omics data, including the requirement for sophisticated data processing
Ali Yetgin
wiley   +1 more source

The High-Redshift Gas-Phase Mass–Metallicity Relation in FIRE-2

open access: yesThe Astrophysical Journal Letters
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

Analysis of carbohydrates and glycoconjugates by matrix‐assisted laser desorption/ionization mass spectrometry: An update for 2021–2022

open access: yesMass Spectrometry Reviews, Volume 44, Issue 3, Page 213-453, May/June 2025.
Abstract The use of matrix‐assisted laser desorption/ionization (MALDI) mass spectrometry for the analysis of carbohydrates and glycoconjugates is a well‐established technique and this review is the 12th update of the original article published in 1999 and brings coverage of the literature to the end of 2022.
David J. Harvey
wiley   +1 more source

Searching for Emission Lines at z > 11: The Role of Damped Lyα and Hints About the Escape of Ionizing Photons

open access: yesThe Astrophysical Journal
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
doaj   +1 more source

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