Results 51 to 60 of about 108,043 (278)
Spectroscopic confirmation of two luminous galaxies at a redshift of 14. [PDF]
Carniani S +44 more
europepmc +2 more sources
First Light: exploring the Spectra of High-Redshift Galaxies in the Renaissance Simulations [PDF]
We present synthetic observations for the first generations of galaxies in the Universe and make predictions for future deep field observations for redshifts greater than 6.
Kirk S. S. Barrow +4 more
semanticscholar +1 more source
Globular clusters as the relics of regular star formation in ‘normal’ high-redshift galaxies [PDF]
We present an end-to-end, two-phase model for the origin of globular clusters (GCs). In the model, populations of stellar clusters form in the high-pressure discs of high-redshift ($z>2$) galaxies (a rapid-disruption phase due to tidal perturbations from
J. Kruijssen
semanticscholar +1 more source
High redshift radio galaxies [PDF]
7 pages including 2 figures. Paper no. 4005-10 in the proceedings of the SPIE International Symposium on 'Astronomical Telescopes and Instrumentation' held in Munich, Germany from 27-31 March ...
openaire +2 more sources
Hot cores: probes of high-redshift galaxies? [PDF]
Updated to correspond to version accepted by ...
Lintott, C.J. +4 more
openaire +4 more sources
The problematic growth of dust in high-redshift galaxies [PDF]
Dust growth via accretion of gas species has been proposed as the dominant process to increase the amount of dust in galaxies. We show here that this hypothesis encounters severe difficulties that make it unfit to explain the observed UV and IR ...
A. Ferrara, S. Viti, C. Ceccarelli
semanticscholar +1 more source
We report the detection of the [O iii ] auroral line in 42 galaxies within the redshift range of 3 < z < 10. These galaxies were selected from publicly available JWST data releases, including the JADES and PRIMAL surveys, and observed using both the low ...
Priyanka Chakraborty +12 more
doaj +1 more source
How passive galaxies form, and the physical mechanisms which prevent star formation over long timescales, are some of the most outstanding questions in understanding galaxy evolution.
Danilo Marchesini +22 more
doaj +1 more source
Why do high-redshift galaxies show diverse gas-phase metallicity gradients? [PDF]
Recent spatially resolved observations of galaxies at z ∼ 0.6–3 reveal that high-redshift galaxies show complex kinematics and a broad distribution of gas-phase metallicity gradients.
Xiangcheng Ma +10 more
semanticscholar +1 more source
Reionisation and High-Redshift Galaxies: The View from Quasar Absorption Lines [PDF]
Determining when and how the first galaxies reionised the intergalactic medium promises to shed light on both the nature of the first objects and the cosmic history of baryons.
G. Becker, J. Bolton, A. Lidz
semanticscholar +1 more source

