Comparing Chemical Abundances of the Damped Lya Systems and Metal-Poor Stars

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dc.creatorProchaska, Jason X.
dc.date2003-10-29
dc.date.accessioned2026-07-07T02:10:56Z
dc.date.available2026-07-07T02:10:56Z
dc.descriptionI briefly draw comparisons between the fields of damped Lya and metal-poor stellar abundances. In particular, I examine their complementary age-metallicity relations and comparisons between the damped Lya and dwarf galaxy abundance patterns. Regarding the latter, I describe a series of problems concerning associating high z damped Lya systems with present-day dwarfs.
dc.description7 pages, 2 figures. To be published in the Proceedings of Joint Discussion 15 of the 2003 IAU, eds. P. Nissen and M. Pettini
dc.identifierhttps://arxiv.org/abs/astro-ph/0310850
dc.identifierhttp://arxiv.org/abs/astro-ph/0310850
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6906
dc.subjectAstrophysics
dc.titleComparing Chemical Abundances of the Damped Lya Systems and Metal-Poor Stars
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