1920
DOI: 10.1007/bf01509078
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(4 citation statements)
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“…The abundance ratios for C, O, Al and Si are all within a factor of two of solar, which suggests that there is not much depletion onto dust grains. We do not see an excess of O with respect to C, as was reported in a few absorption systems (Vogel & Reimers 1993).…”
Section: Discussionsupporting
confidence: 86%
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“…The abundance ratios for C, O, Al and Si are all within a factor of two of solar, which suggests that there is not much depletion onto dust grains. We do not see an excess of O with respect to C, as was reported in a few absorption systems (Vogel & Reimers 1993).…”
Section: Discussionsupporting
confidence: 86%
“…First, we believe that the gas abundances which we measure are close to the total abundances, because the ratio of Aluminum to other elements is near cosmic, and Al is a refractory element which depletes very readily, like Chromium, in the interstellar medium. Second, we do not see the enhancement of O with respect to C of [O/C] ≃ 0.5 − 0.9 reported in three partial Lyman limit systems by Reimers et al 1992 andReimers 1993; we measure [O/C] = −0.06 for observed ions and [O/C] ≃ 0.2 after ionization corrections, which is consistent with solar abundances. We see C II * (λ1335) offset by 15 km s −1 with respect to C II(λ1334), presumably because the gas density varies from 2 -8 cm −3 with changing velocity in the DLA system.…”
supporting
confidence: 82%
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