Results 81 to 90 of about 4,926,824 (288)
In this paper, we present the Heavy Metal Survey, which obtained ultradeep medium-resolution spectra of 21 massive quiescent galaxies at 1.3 < z < 2.3 with Keck/LRIS and MOSFIRE.
Mariska Kriek+16 more
doaj +1 more source
Star Formation for Predictive Primordial Galaxy Formation
The elegance of inflationary cosmology and cosmological perturbation theory ends with the formation of the first stars and galaxies, the initial sources of light that launched the phenomenologically rich process of cosmic reionization. Here we review the
Milosavljevic, Milos+1 more
core +1 more source
Locally Biased Galaxy Formation and Large Scale Structure [PDF]
We examine the influence of the morphology-density(MD) relation and a wide range of simple models for biased galaxy formation on statistical measures of large scale structure.
Abell G. O.+28 more
core +3 more sources
nIFTy cosmology: comparison of galaxy formation models [PDF]
We present a comparison of 14 galaxy formation models: 12 different semi-analytical models and 2 halo occupation distribution models for galaxy formation based upon the same cosmological simulation and merger tree information derived from it.
A. Knebe+35 more
semanticscholar +1 more source
Gas-Rich Companions of Isolated Galaxies [PDF]
We have used the VLA to search for gaseous remnants of the galaxy formation process around six extremely isolated galaxies. We found two distinct HI clouds around each of two galaxies in our sample (UGC 9762 & UGC 11124).
Byrd G. G.+6 more
core +4 more sources
The Formation of the First Galaxies
Ph. D. Thesis, University of Heidelberg, 2009, 212 pages, 55 figures, pdf available at http://www.ita.uni-heidelberg.de/~tgreif/thesis.shtml?lang ...
openaire +4 more sources
The EAGLE simulations of galaxy formation: the importance of the hydrodynamics scheme [PDF]
We present results from a subset of simulations from the "Evolution and Assembly of GaLaxies and their Environments" (EAGLE) suite in which the formulation of the hydrodynamics scheme is varied.
M. Schaller+11 more
semanticscholar +1 more source
Diffuse Light in Milky Way–like Haloes
We investigate the diffuse light (DL) content of dark matter haloes in the mass range $11.5\leqslant \mathrm{log}{M}_{\mathrm{halo}}\leqslant 13$ , a range that also includes the dark matter halo of the Milky Way, taking advantage of a state-of-the-art ...
Emanuele Contini+4 more
doaj +1 more source
Mapping Global Star Formation in the Interacting Galaxy Pair Arp32 [PDF]
A multi-wavelength set of photometric data including UV (GALEX), optical, near-IR, infrared (Spitzer) and radio (VLA 20cm) images and spectroscopic observations are used to map the dust-obscured and unobscured star formation in the galaxy pair Arp 32 ...
Appleton, P.+7 more
core
How do galaxies get their baryons?
Understanding how galaxies obtain baryons, their stars and gas, over cosmic time is traditionally approached in two different ways - theoretically and observationally.
Conselice, Christopher J.
core +1 more source