Titlebook: Cold Gas at High Redshift; Proceedings of a Wor M. N. Bremer,P. P. Werf,C. L. Carilli Conference proceedings 1996 Kluwer Academic Publisher

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https://doi.org/10.1007/978-3-030-35272-1ion of gas within a merging hierarchy of dark matter halos. A simple Kennicutt law of star formation for disks, based on a single-fluid gravitational stability model, is introduced. Since the gas supply in the disk is regulated by infall from the surrounding halo, the gas is always maintained at a c

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Serial Rings with Krull Dimension,ds and argue by comparison with cosmological simulations that Lyman . forest observations show the signs of ongoing gravitational structure formation at high redshift. The departures of observed line profiles from thermal Voigt profiles (caused by bulk motion of infalling gas and compressional heati

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,Two’s Complement Multiplication,surveying instruments. Pointed observations of galaxies in the nearest clusters of galaxies, such as Virgo, Coma and A1367, reveal shrunken H I disks in the cluster cores and detailed studies of the H I surface density distribution make it possible to identify the various gas removal processes at wo

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Stewart G. Smith,Peter B. Denyer those of galaxies found in a survey of regions of mean cosmic density. The Boötes survey covers 1100 Mpc., or ~ 1% of the volume of the void and consists of 24 cubes of typically 2 Mpc × 2 Mpc X 1280 km s., centered on optically known galaxies. Sixteen targets were detected in HI; 18 previously unc

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978-94-010-7273-1Kluwer Academic Publishers 1996

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Jessica Woodhams,Clive Hollin,Ray Bullstructures of small overdensity. It is argued that the observed absorbers should be preferentially located in underdense regions of the universe and should typically expand faster than the Hubble flow.

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Are the Lyman Alpha Forest “Clouds” Expanding Pancakes?structures of small overdensity. It is argued that the observed absorbers should be preferentially located in underdense regions of the universe and should typically expand faster than the Hubble flow.