Results 31 to 40 of about 147,516 (226)

Formation of globular cluster candidates in merging proto-galaxies at high redshift: a view from the FIRE cosmological simulations [PDF]

open access: yes, 2017
Using a state-of-the-art cosmological simulation of merging proto-galaxies at high redshift from the FIRE project, with explicit treatments of star formation and stellar feedback in the interstellar medium, we investigate the formation of star clusters ...
Ji-hoon Kim   +28 more
semanticscholar   +1 more source

Large Disklike Galaxies at High Redshift [PDF]

open access: yesThe Astrophysical Journal, 2003
LaTeX, 5 pages, 2 figures, 1 table.
Labbé, Ivo   +13 more
openaire   +5 more sources

The MUSE Hubble Ultra Deep Field Survey: II. Spectroscopic redshifts and comparisons to color selections of high-redshift galaxies [PDF]

open access: yes, 2017
We have conducted a two-layered spectroscopic survey (1′ × 1′ ultra deep and 3′ × 3′ deep regions) in the Hubble Ultra Deep Field (HUDF) with the Multi Unit Spectroscopic Explorer (MUSE).
H. Inami   +30 more
semanticscholar   +1 more source

Cosmology at high redshift — a probe of fundamental physics [PDF]

open access: yesJournal of Cosmology and Astroparticle Physics, 2021
An observational program focused on the high redshift ...
N. Sailer   +3 more
semanticscholar   +1 more source

Is There a Missing Galaxy Problem at High Redshift? [PDF]

open access: yesThe Astrophysical Journal, 2004
We study the evolution of the global stellar mass density in a Lambda cold dark matter universe using two different types of hydrodynamical simulations (Eulerian TVD and SPH) and the analytical model of Hernquist & Springel (2003). We find that the theoretical calculations all predict both a higher stellar mass density at z~3 than indicated by ...
Nagamine, Kentaro   +4 more
openaire   +5 more sources

High-Redshift Radio Galaxies [PDF]

open access: yesHighlights of Astronomy, 1995
Radio galaxies are unique cosmological probes. As with radio-loud quasars, the presence of luminous radio continuum and optical line emission enable radio galaxies to be observed and recognized at large distances, up to z = 4.2. However, unlike the situation for most quasars, their optical emission can be spatially resolved from the ground and studied ...
openaire   +1 more source

The Extinction Law in High‐Redshift Galaxies [PDF]

open access: yesThe Astrophysical Journal, 2004
We estimate the dust extinction laws in two intermediate redshift galaxies. The dust in the lens galaxy of LBQS1009-0252, which has an estimated lens redshift of zl~0.88, appears to be similar to that of the SMC with no significant feature at 2175 A.
Munoz, J. A.   +4 more
openaire   +2 more sources

GRB Host Galaxies: An Unbiased Sample [PDF]

open access: yes, 2011
We describe the current status and recent results from our Swift/VLT legacy survey, a VLT Large Programme aimed at characterizing the host galaxies of a homogeneously selected sub-sample of Swift GRBs.
Milvang-Jensen, Bo   +6 more
core   +1 more source

The formation of high-redshift submillimetre galaxies [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2010
MNRAS Accepted; Revised version includes expanded discussion of simulated radio properties of ...
Narayanan, Desika   +6 more
openaire   +4 more sources

Relativistic jet feedback in high-redshift galaxies – I. Dynamics [PDF]

open access: yes, 2016
We present the results of three dimensional relativistic hydrodynamic simulations of interaction of AGN jets with a dense turbulent two-phase interstellar medium, which would be typical of high redshift galaxies.
D. Mukherjee   +3 more
semanticscholar   +1 more source

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