The Core of the Great Attractor; Is it behind the Southern Milky Way?
The nature and the extent of the Great Attractor has been the subject of much debate, not in the least
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Great Wall
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1.65 micron (H-band) surface photometry of galaxies. V: Profile decomposition of 1157 galaxies
We present near-infrared H-band (1.65 micron) surface brightness profile decomposition for 1157 galaxies in five nearby clusters of galaxies: Coma,
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A Constraint on the Distance Scale to Cosmological Gamma--Ray Bursts
If gamma-ray bursts have a cosmological origin, the sources are expected to trace the large-scale structure of luminous matter in
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A Search For Large-Scale Structure at High Redshift
We present new and exciting results on our search for large-scale structure at high redshift. Specifically, we have just completed
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Fractal Approach to Large-Scale Galaxy Distribution
We present a review of the history and the present state of the fractal approach to the large-scale distribution of
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The ESO Slice Project (ESP) galaxy redshift survey: I. Description and First Results
The ESO Slice Project (ESP) is a galaxy redshift survey we have recently completed as an ESO Key-Project. The ESP
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The Local Ly-alpha forest: Association of absorbers with galaxies, voids, and superclusters
We describe recent discoveries of low column density [N(HI) < 10^14.5 cm^-2] H I Ly-alpha absorbers made with the Hubble
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The Local Ly-alpha Forest: HI in Nearby Intergalactic Space
Detecting HI using redshifted Ly-alpha absorption lines is 1e6 times more sensitive than using the 21cm emission line. We review
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Numerical Domain Wall Type Solutions in phi**4 Theory
The well known domain wall type solutions are nowadays of great physical interest in classical field theory. These solutions can
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Large-Scale Structures behind the Southern Milky Way in the Great Attractor Region
A deep optical galaxy search behind the southern Milky Way and a subsequent redshift survey of the identified obscured galaxies
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Dusty Tori of Seyfert Nuclei
Dusty tori around active galactic nuclei (AGNs) play an important role in the classification of Seyfert galaxies. Therefore, physical properties
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The Core of the Great Attractor
The nature and extent of the Great Attractor (GA) has been the subject of much debate in the past decade,
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