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astro-ph1997

Abundances of Heavy Elements and CO Molecules in High Redshift Damped Lyman-alpha Galaxies

Limin Lu, Wallace L. W. Sargent, Thomas A. Barlow

Damped Lyman-alpha systems seen in spectra of background quasars are generally thought to represent high redshift counterparts of present-day galaxies. We summarize observations of…

astro-ph1997

Abundances in Damped Lyman-alpha Systems and Chemical Evolution of High Redshift Galaxies

Limin Lu, Wallace L. W. Sargent, Thomas A. Barlow

Recent abundance measurements in damped Lyman-alpha galaxies, supplemented with unpublished Keck observations, are discussed. The metallicity distribution with cosmic time is exami…

astro-ph1997

Partial Coverage and Time Variability of Narrow-Line Intrinsic QSO Absorption Systems

Thomas A. Barlow, F. Hamann, W. L. W. Sargent

It is possible to distinguish ``intrinsic'' absorption systems (gas clouds within the quasar environment) from ``intervening'' systems (gas clouds unrelated to the quasar phenomeno…

astro-ph1997

High-Velocity Narrow-Line Absorbers in QSOs

F. Hamann, T. Barlow, R. D. Cohen +2

We discuss the identification and kinematics of intrinsic narrow-line absorbers in three QSOs. The line-of-sight ejection velocities in the confirmed intrinsic systems range from 1…

astro-ph1997

Initial Chemical Enrichment in Galaxies

Limin Lu, Wallace L. W. Sargent, Thomas A. Barlow

We present evidence that damped Lyman-alpha galaxies detected in spectra of quasars may not have started forming stars until the redshift z~3. If damped Lyman-alpha absorbers are t…