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Pruning the Lyman   forest of Q1331 + 170

Varsha P. KulkarniK. HuangR. F. GreenJill BechtoldD. E. WeltyD. G. York

1996Monthly Notices of the Royal Astronomical SocietyPhysics and Astronomy被引 40

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摘要

We present a study of the Lyman α forest of the QSO 1331 +170 in the range 1.67 <zabs < 2.10 at 18 km s−1 resolution. Our analysis includes a careful search for previously unidentified heavy-element systems, and incorporates detailed deblending of Lyα forest lines from heavy-element lines. Various statistical properties of Lyα forest lines, such as distributions of equivalent widths, H I column densities, Doppler parameters and pair-velocity separations, are computed. The effect on these properties of employing different limiting approaches to heavy- eiement deblending, and profile-fitting of the lines, is illustrated. Our data suggest that the NH distribution may not be fitted adequately by a single power law, i.e., that there may be a relative deficit of strong lines as compared with the predictions of a single power law. However, larger samples are required to verify this deficit. The median b value is ≈ 32 km s−1 No significant correlation is observed between NH and b. An excess on the scale of ∼100 km s−1 is seen in the pair-velocity correlations, at the level of ∼ 2.6σ for the conservative sample and at the level of ∼ 4.9(7.for the less conservative sample. Marginal excess correlation is seen in both the samples at the ≿2σ level on scales of ∼800–1000 km s−1, and also on scales of ∼6000 km s−1.

引用本文(GB/T 7714)

Varsha P. Kulkarni, K. Huang, R. F. Green, 等. Pruning the Lyman   forest of Q1331 + 170[J]. Monthly Notices of the Royal Astronomical Society, 1996.

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DOI:https://doi.org/10.1093/mnras/279.1.197

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