Distinct abundance patterns in multiple damped Lyα galaxies

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dc.contributor.authorLopez, S
dc.contributor.authorEllison, SL
dc.date.accessioned2025-01-21T01:09:24Z
dc.date.available2025-01-21T01:09:24Z
dc.date.issued2003
dc.description.abstractFollowing our previous work on metal abundances of a double damped Lyalpha system with a line-of-sight separation similar to2000 km s(-1) (Ellison & Lopez 2001), we present VLT UVES abundances of 3 new systems spanning a total of similar to6000 km s-1 at z similar to 2.5 toward the southern QSO CTQ247. These abundances are supplemented with echelle observations of another "double" damped Lyalpha system in the literature. We propose a definition in terms of velocity shift of the sub-class "multiple damped Lyalpha system", which is motivated by its possible connection with large-scale structure. We find that the abundance ratio [S/Fe] is systematically low in multiple systems compared with single systems, and with a small scatter. The same behavior is found in 2 more single DLA systems taken from the literature that show evidence of belonging to a galaxy group. Although [Si/Fe] ratios are also generally lower in multiple DLAs than in single DLAs, the effect is less striking since the scatter is larger and there are a number of low [Si/Fe] DLAs in the literature. We suggest that this can be explained with a combination of detection bias and, to a lesser extent, the scatter in ionization corrections for different absorbers. We investigate whether consistently low alpha/Fe ratios could be due to dust depletion or ionization corrections and find that the former effect would emphasize the observed trend of low alpha/Fe in multiple systems even further. Ionization may have a minor effect in some cases, but at a level that would not change our conclusions. We thus conclude that the low alpha/Fe ratios in multiple DLAs have a nucleosynthetic origin and suggest that they could be explained by reduced star formation in multiple damped Lyalpha systems, possibly due to environmental effects. There seems to be independent evidence for this scenario from the mild odd-even effect and from the relatively high N/alpha ratios we observe in these multiple systems.
dc.fuente.origenWOS
dc.identifier.doi10.1051/0004-6361:20030403
dc.identifier.eissn1432-0746
dc.identifier.issn0004-6361
dc.identifier.urihttps://doi.org/10.1051/0004-6361:20030403
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/96579
dc.identifier.wosidWOS:000182678800023
dc.issue.numero2
dc.language.isoen
dc.pagina.final584
dc.pagina.inicio573
dc.revistaAstronomy & astrophysics
dc.rightsacceso restringido
dc.subjectquasars : general
dc.subjectquasars : absorption lines
dc.subjectquasars : individual : CTQ247
dc.subjectgalaxies : evolution
dc.subjectgalaxies : clusters : general
dc.titleDistinct abundance patterns in multiple damped Lyα galaxies
dc.typeartículo
dc.volumen403
sipa.indexWOS
sipa.trazabilidadWOS;2025-01-12
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