Statistical characteristics of the observed metal systems and problems of reionization
M. Demia\'nski, A.G. Doroshkevich

TL;DR
This study examines metal systems in quasar spectra to understand their properties, distribution, and implications for cosmic reionization, revealing thermal broadening dominance, typical protogalaxy sizes, and the limited role of stars in reionization.
Contribution
It provides detailed analysis of metal system properties, their spatial distribution, and implications for reionization, highlighting the need for additional UV sources beyond stellar contributions.
Findings
Metal Doppler parameters indicate thermal broadening dominance.
Metal systems are located in regions of 0.1-0.25h^{-1} Mpc, typical of protogalaxies.
Metal abundances suggest stars alone cannot account for reionization.
Abstract
We analyze basic properties of about 200 metal systems observed in high resolution spectra of 9 quasars by Boksenberg, Sargent & Rauch (2003). The measured Doppler parameters for the hydrogen and carbon lines are found to be different by a factor what indicates the domination of the thermal broadening and high degree of relaxation for majority of the observed metal systems. The analysis of the mean separation of the metal systems confirms that they can be located in regions with the typical proper size Mpc what corresponds to the typical sizes of protogalaxies with the baryonic masses . The metal abundances observed at redshifts within both IGM and galaxies are found to be quite similar to each other what indicates the strong interaction of young galaxies with the IGM and the important role of…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsAdvanced Materials Characterization Techniques · Material Properties and Failure Mechanisms
