QSO Absorption Lines, Gaseous Infall and Star Formation

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dc.creatorCirkovic, Milan M.
dc.creatorSamurovic, Srdjan
dc.creatorMilosevic-Zdjelar, Vesna
dc.date2000-10-12
dc.date.accessioned2026-07-07T01:55:57Z
dc.date.available2026-07-07T01:55:57Z
dc.descriptionWe investigate the impact of recent observational advances in research on the gaseous content of the universe on our knowledge of star formation histories of disk galaxies. Several contemporary surveys indicate that large quantities of gas which has not been astrated or has been astrated only weakly are bound to galaxies at later epochs ($z\le 1$).
dc.description2 pages, no figures. Proceedings of the conference "Galaxy Disks and Disk Galaxies", ASP Conference Series, eds. J.G. Funes, S.J. and E.M. Corsini
dc.identifierhttps://arxiv.org/abs/astro-ph/0010247
dc.identifierhttp://arxiv.org/abs/astro-ph/0010247
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1832
dc.subjectAstrophysics
dc.titleQSO Absorption Lines, Gaseous Infall and Star Formation
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