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Cosmology with Galaxies at High Redshifts
1991Following some remarks on the methodology of the classical cosmological tests, recent observations of galaxies at high redshift are examined to see whether they place any constraints on the cosmological models. It is concluded that, at least at present, they do not.
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Galaxy Morphology at High Redshift
2014The morphology of galaxies at high redshift ranges from elliptical and spiral to clumpy, including chains, clump clusters, doubles and tadpoles. Clumpy galaxies observed in the Hubble Ultra Deep Field at redshifts z = 1–5 contain star-forming complexes that are hundreds of times more massive than those forming in local galaxies, reflecting the more ...
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Simulations of the formation, evolution and clustering of galaxies and quasars
Nature, 2005Volker Springel +2 more
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Properties of galaxies reproduced by a hydrodynamic simulation
Nature, 2014Mark Vogelsberger +2 more
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High molecular gas fractions in normal massive star-forming galaxies in the young Universe
Nature, 2010Linda Tacconi +2 more
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Strangulation as the primary mechanism for shutting down star formation in galaxies
Nature, 2015Roberto Maiolino
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Systematic variation of the stellar initial mass function in early-type galaxies
Nature, 2012Michele Cappellari +2 more
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Galaxies at redshifts 5 to 6 with systematically low dust content and high [C ii] emission
Nature, 2015Peter Capak +2 more
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Modeling the Panchromatic Spectral Energy Distributions of Galaxies
Annual Review of Astronomy and Astrophysics, 2013Charlie Conroy
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