Results 11 to 20 of about 461,621 (314)
The clustering evolution of the galaxy distribution [PDF]
Monthly Notices of the Royal Astronomical Society, 2001 18 pages, 9 figures. Submitted to MNRAS. High-resolution copies of the colour figures can be found at http://www.astro.caltech.edu/~abenson/Mocks/mocks ...
Benson, A.J. +4 more
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Evolution of galaxy clustering [PDF]
Monthly Notices of the Royal Astronomical Society, 1998 Four pages, 1 figure.
openaire +4 more sources
The GALEX Extended Mission: Surveying UV Tracers of the Hidden Side of Galaxy Evolution [PDF]
, 2010 The Galaxy Evolution Explorer (GALEX) continues its surveys of the ultraviolet sky. GALEX surveys have supported the following galaxy evolution investigations: calibrating UV as a star formation rate tracer, using wide and deep surveys to measure star ...
Martin, D. Christopher
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An analysis of the evolving comoving number density of galaxies in hydrodynamical simulations [PDF]
, 2015 The cumulative comoving number-density of galaxies as a function of stellar mass or central velocity dispersion is commonly used to link galaxy populations across different epochs.
Griffen, Brendan F. +12 more
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Numerical simulations of galaxy evolution in cosmological context [PDF]
, 2008 Large volume cosmological simulations succeed in reproducing the large-scale structure of the Universe. However, they lack resolution and may not take into account all relevant physical processes to test if the detail properties of galaxies can be ...
Bournaud +6 more
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The Morphological Evolution of Galaxies
Science, 2001 Many galaxies have taken on their familiar appearance relatively recently. In the distant Universe, galaxy morphology deviates significantly (and systematically) from that of nearby galaxies at redshifts (z) as low as 0.3. This corresponds to a time ∼3.5 × 109years in the past, which is only ∼25% of the present age of the Universe.
Roberto Abraham, Sidney van den Bergh
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The Effect of Gas Fraction on the Morphology and Time-scales of Disc Galaxy Mergers [PDF]
, 2009 Gas-rich galaxy mergers are more easily identified by their disturbed morphologies than mergers with less gas. Because the typical gas fraction of galaxy mergers is expected to increase with redshift, the under-counting of low gas-fraction mergers may ...
Abazajian +73 more
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The Morphological Evolution of Field Galaxies [PDF]
Symposium - International Astronomical Union, 1995 I review two observational programs which, together, promise to unravel the detailed astrophysical evolution of normal field galaxies over the last 5-7 Gyr. Systematic ground-based spectroscopy of faint galaxies have revealed an increasing faint end slope for the luminosity function with redshift.
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Exploring Galaxy Evolution from Infrared Number Counts and Cosmic Infrared Background [PDF]
, 2000 Recently reported infrared (IR) galaxy number counts and cosmic infrared background (CIRB) all suggest that galaxies have experienced a strong evolution sometime in their lifetime.
Hirashita, Hiroyuki +6 more
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Evolution of galaxies in clusters
The Astrophysical Journal, 1994 33 pages, normal ...
Joseph Silk, Stephane Charlot
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