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Showing 1997Show all

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astro-ph1997

A High Deuterium Abundance at z=0.7; Evidence for Cosmic Inhomogeneity?

J. K. Webb, R. F. Carswell, K. M. Lanzetta +3

Recent HST/GHRS observations of the z = 0.7010 absorber toward the QSO 1718+4807 (selected because of apparently ideal characteristics for measuring D/H) yield a D/H significantly…

astro-ph1997

Limits on the Variability of Physical Constants

M. J. Drinkwater, J. K. Webb, J. D. Barrow +1

We have compared the frequency of high-redshift Hydrogen HI 21 cm absorption with that of associated molecular absorption in two quasars to place new (1 sigma) upper limits on any…

astro-ph1997

The Gaseous Extent of Galaxies and the Origin of \lya Absorption Systems at z < 1

H. -W. Chen, K. M. Lanzetta, J. K. Webb +1

We present initial results of a program to obtain and analyze HST WFPC2 images of galaxies in fields of HST spectroscopic target QSOs. The goal of the program is to investigate how…

astro-ph1997

The Galaxy-Absorber Cross-Correlation Function

Kenneth M. Lanzetta, John K. Webb, Xavier Barcons

We describe an analysis of the galaxy-absorber cross-correlation function as a function of velocity separation, impact parameter separation, and absorber Lyman alpha equivalent wid…

astro-ph1997

Lyman-alpha absorbers arising in galaxy clusters

A. Ortiz-Gil, K. M. Lanzetta, J. K. Webb +1

We present here new GHRS observations of Lyman-alpha absorption lines associated with groups or clusters toward the QSOs 1545+2101 and 0850+4400. In the first case we have identifi…

astro-ph1997

Structure in the Lyman-Alpha Forest

J. Liske, J. K. Webb

The spatial distribution of Ly-alpha forest absorption systems toward a group of 8, closely spaced QSOs has been analysed and evidence for large scale structure has been found at <…