Results 1 to 10 of about 558 (138)
Morphological Classification of High Redshift Galaxies [PDF]
Astrophysics and Space Science, 2001 4 pages, 3 encapsulated figures. Proceedings of the Euroconference "The Evolution of Galaxies.I- Observational clues." held in Granada (Spain), 23-27 May, 2000.
Pignatelli, E., Fasano, G.
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Galaxies at High Redshift [PDF]
Astrophysics and Space Science, 1999 Within just the last few years, we have advanced from knowing only a few galaxies at z>2 to having redshifts for nearly 1000 z~2-5 objects. The majority of this sample has been detected through the photometric ``drop-out'' technique used so successfully by Steidel and his collaborators. In addition, a handful of objects have already been detected at
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The circumgalactic medium of high-redshift galaxies [PDF]
Monthly Notices of the Royal Astronomical Society: Letters, 2014 Abstract We study the properties of the circumgalactic medium (CGM) of high-z galaxies in the metal enrichment simulations presented in Pallottini et al. At z = 4, we find that the simulated CGM gas density profiles are self-similar, once scaled with the virial radius of the parent dark matter halo.
PALLOTTINI, ANDREA +2 more
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, 1998 To appear in "Large Scale Structure: Tracks and Traces", Proceedings of the 12th Potsdam Cosmology Workshop, eds. V. M"uller, S. Gottl"ober, J. P. M"ucket, J. Wambsganss, (Singapore: World Scientific), 1998. 9 LaTeX pages, including 5 figures.
Yahil, A. +2 more
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Galaxy bulges at mid- and high-redshift [PDF]
Proceedings of the International Astronomical Union, 2007 AbstractBulges are a major galaxy component in the nearby universe, and are one of the primary features that differentiates and defines galaxies. The origin of bulges can be directly probed in part by examining distant galaxies to search for high redshift bulges, and to study the properties of bulges in formation.
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ON THE SHAPES AND STRUCTURES OF HIGH-REDSHIFT COMPACT GALAXIES [PDF]
The Astrophysical Journal, 2012 9 pages, 3 figure, accepted for publication in ...
Chevance, Melanie +7 more
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High Redshift Radio Galaxies with the VLT [PDF]
, 1997 The study of high-$z$ radio galaxies (HZRGs) has matured considerably during the last decade. Large numbers of $z>2$ radio galaxies have been found and have been studied in considerable detail. In this review we will address the importance of the VLT for studies of samples of distant radio galaxies.
Röttgering, H. J. A., Miley, G. K.
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Hot cores: probes of high-redshift galaxies? [PDF]
Monthly Notices of the Royal Astronomical Society, 2005 Updated to correspond to version accepted by ...
Lintott, C.J. +4 more
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THE PREMATURE FORMATION OF HIGH-REDSHIFT GALAXIES [PDF]
The Astronomical Journal, 2014 Accepted for publication in the Astronomical ...
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The visibility of high-redshift galaxies [PDF]
Monthly Notices of the Royal Astronomical Society, 1990 The most visible galaxies (those which have the largest apparent sizes and isophotal luminosities when seen at a given distance) are those with a particular observed surface brightness. Extending this argument to high-redshift galaxies, it is clear that this optimum surface brightness moves progressively to brighter intrinsic surface brightnesses, so ...
S. Phillipps, J. I. Davies, M. J. Disney
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