On the Origin of Nitrogen in Damped Ly-alpha Systems

dc.creatorHenry, R. B. C.
dc.creatorProchaska, Jason X.
dc.date2002-11-22
dc.date.accessioned2026-07-07T02:06:31Z
dc.date.available2026-07-07T02:06:31Z
dc.descriptionRecent measurements of nitrogen and alpha elements in over 20 damped Ly-alpha systems (DLA) are compared with similar measurements for numerous emission line objects and stars. It is found that the DLA distribution in the N/alpha-alpha/H plane is bimodal, where most sample DLAs fall along the N/alpha plateau defined at low Z by dwarf irregulars, while a small group possesses N/alpha values roughly 0.7 dex less than those on the plateau at similar alpha/H values. We demonstrate with chemical evolution models that a top-heavy or truncated IMF can account for the low N in this second group.
dc.description7 pages, in ``CNO in the Universe,'' ASP Conference Series, in press edited by C. Charbonnel, D. Schaerer, and G. Meynet
dc.identifierhttps://arxiv.org/abs/astro-ph/0211512
dc.identifierhttp://arxiv.org/abs/astro-ph/0211512
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5390
dc.subjectAstrophysics
dc.titleOn the Origin of Nitrogen in Damped Ly-alpha Systems
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