Astronomy and Astrophysics – Astrophysics
Scientific paper
1997-08-28
Astronomy and Astrophysics
Astrophysics
4 LaTeX pages, with 2 encapsulated PostScript figures, uses conf_iap.sty (included). To appear in the Proceedings of the 13th
Scientific paper
We have analyzed the clustering of C IV and Mg II absorption-line systems on comoving scales from 1 to 16 \hMpc, using an extensive catalog of heavy-element QSO absorbers with mean redshift 2.2 (C IV) and 0.9 (Mg II). For the C IV sample as a whole, the absorber line-of-sight correlation function is well fit by a power law of the form $\xi(r)=(r_0/r)^\gamma$, with maximum-likelihood values of $\gamma = 1.75 ^{+0.50}_{-0.70}$ and comoving $r_0 = 3.4 ^{+0.7}_{-1.0}$ \hMpc ($q_0=0.5$). This clustering is of the same form as that for galaxies and clusters at low redshift, and of amplitude such that absorbers are correlated on scales of clusters of galaxies. We also trace the evolution of the mean amplitude $\xi_0(z)$ of the correlation function from $z=3$ to $z=0.9$. We find that, when parametrized as $\xi_0(z)\propto (1+z)^{-(3+\epsilon)+\gamma}$, the amplitude grows rapidly with decreasing redshift, with maximum-likelihood value for the evolutionary parameter of $\epsilon = 2.05 \pm 1.0$. The rapid growth seen in the clustering of absorbers is consistent with gravitationally induced growth of perturbations.
Quashnock Jean M.
Vanden Berk Daniel E.
No associations
LandOfFree
The Clustering of C IV and Mg II Absorption-Line Systems does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The Clustering of C IV and Mg II Absorption-Line Systems, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Clustering of C IV and Mg II Absorption-Line Systems will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-519452