Initial Chemical Enrichment in Galaxies

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dc.creatorLu, Limin
dc.creatorSargent, Wallace L. W.
dc.creatorBarlow, Thomas A.
dc.date1997-01-30
dc.date.accessioned2026-07-07T02:22:50Z
dc.date.available2026-07-07T02:22:50Z
dc.descriptionWe 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 the progenitors of disk galaxies, then the above result may indicate that star formation in galactic disks first began at z~3.
dc.descriptionLaTeX, 1 PS figure, to appear in the Proceedings of the 18th Texas Symposium (1997)
dc.identifierhttps://arxiv.org/abs/astro-ph/9701241
dc.identifierhttp://arxiv.org/abs/astro-ph/9701241
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11027
dc.subjectAstrophysics
dc.titleInitial Chemical Enrichment in Galaxies
dc.typetext

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