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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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Stacey L. Shipley,Bruce A. Arrigobeing undertaken by ISO. The depth and areal coverage were designed to complement the various Guaranteed Time surveys. The main science thrust is to explore star formation in galaxies to a much higher redshift than was probed by IRAS. We expect to detect around 8000 extragalactic objects and a simil
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Compulsive-Repetitive OffendersTo investigate their redshifts, star formation characteristics, optical morphologies, and evolution, we have used the 10-meter Keck telescope to obtain . broad-band images and optical spectra of a complete sample of .Jy sources detected in three fields at the VLA. In one field, only 1 of 16 sources
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Erica P. Hodges,Kristine M. Jacquind tunnels. Zel’dovich (1970) showed that gravitational instability in an expanding universe can create such structures from generic random initial conditions. Zeldovich’s analysis was originally used to describe the first collapse in “top-down” scenarios like the hot dark matter model, which have a
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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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https://doi.org/10.1007/978-3-030-35272-1 formed by the process of gravitational instability. The 1-D correlation function (along the line-of-sight) is equal to the 3-D function, so long as the spatial separation of clouds is much greater than their size. Observations of close quasar pairs suggest that this may not be the case. We present
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