Results 111 to 120 of about 90,215 (275)
Dusty Star-Forming Galaxies at High Redshift
, 2014 Far-infrared and submillimeter wavelength surveys have now established the important role of dusty, star-forming galaxies (DSFGs) in the assembly of stellar mass and the evolution of massive galaxies in the Universe.
Casey, Caitlin M. +2 more
core +1 more source
γ-ray/infrared luminosity correlation of star-forming galaxies [PDF]
, 2020 P. Kornecki +5 more
openalex +1 more source
Short‐Term Effect of Mars‐Like Radiation on Carbon and Oxygen Isotope Compositions of Carbonates
Journal of Geophysical Research: Planets, Volume 131, Issue 1, January 2026.Abstract The stable isotope composition of carbonates records the environmental formation conditions and can indicate potential biosignatures if formed biologically. Martian meteorite carbonates display unusually high δ13C values, not explained using known terrestrial processes.
Nicolas Randazzo +5 more
wiley +1 more source
Dynamic Chiral Plasmonic Systems‐Based on Spiropyran Derivatives and Gold Nanorods
Advanced Materials Interfaces, Volume 12, Issue 23, December 8, 2025.Soft chiral plasmonic nanocomposites are prepared by embedding gold nanorods into spiropyran‐based supramolecular gels. The system self‐assembles into helical structures, enabling plasmonic circular dichroism. When illuminated with UV light spiropyran–merocyanine isomerization occurs, inducing reversible nanoscale reorganization and modulation of the ...
Ewelina Tomczyk +4 more
wiley +1 more source
The distribution and lifetime of powerful radio galaxies as a function of environment and redshift
Scientific Reports, 2018 Correlations between jet power and active time for z
David Garofalo +2 more
doaj +1 more source
The infrared properties of star-forming galaxies, primarily as determined by the Infrared Astronomy Satellite (IRAS), are compared to X-ray, optical, and radio properties.
Weedman, Daniel W.
core +1 more source
ISO Spectroscopy of Ultraluminous Infrared Galaxies
Astrophysics and Space Science, 1999 Spectroscopy from the Infrared Space Observatory ISO has for the first timeprovided the sensitivity to exploit the diagnostic power ofmid-infrared fine structure lines and PAH features for the study ofultraluminous infrared galaxies (LIR >1012 L ⊙). We report on observations obtainedwith SWS, ISOPHOT-S, and the CVF option of ISOCAM.
Lutz, D +7 more
openaire +1 more source
Near-infrared imaging of interacting galaxies
The Astrophysical Journal, 1990 Galaxy-galaxy interactions are known to cause dramatic changes in morphology and at the same time often induce large bursts of star formation activity. While optical images are sufficient to reveal the overall morphological peculiarities of these systems, they suffer from several problems, the greatest of which is obscuration by dust within the ...
H. A. Bushouse, M. W. Werner
openaire +1 more source
The QSO — Ultraluminous Infrared Galaxies Connection [PDF]
, 2001 For the past several years, our group has pursued a vigorous ground-based program aimed at understanding the nature of ultraluminous infrared galaxies. We recently published the results from a optical/near-infrared spectroscopic survey of a large statistically complete sample of ultraluminous infrared galaxies (the "IRAS 1-Jy sample").
Veilleux, S. +2 more
openaire +2 more sources
The physiology of survival: Space
Experimental Physiology, EarlyView.
Damian M. Bailey, Angelique van Ombergen
wiley +1 more source