Hostname: page-component-6bb9c88b65-spzww Total loading time: 0 Render date: 2025-07-26T15:07:24.106Z Has data issue: false hasContentIssue false

Gas in cosmic voids*

Published online by Cambridge University Press:  19 July 2016

P M Gondhalekar
Affiliation:
Rutherford Appleton Laboratory, Chilton, Didcot, Oxon, OX11 0QX, United Kingdom
N Brosch
Affiliation:
Wise Observatory, University of Tel Aviv, Tel Aviv 69978, Israel

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Absorption lines at the redshifts of cosmic voids in Perseus-Pisces and Böotes have been detected in the ultraviolet spectra of background quasars. The detection of Si IV and C IV lines besides Ly α suggests chemical enrichment of gas in the voids. Additional observations of three sight-lines through the void in the Böotes suggests that the gas in the void is clumped in large clouds.

Information

Type
VI. Quasars as Probes of the Intervening Medium
Copyright
Copyright © Reidel 1986 

References

Brosch, N & Greenberg, J M, 1983. Astrophys Sp Sci 90, 457.Google Scholar
Brosch, N & Gondhalekar, P M, 1984. Astron Astrophys 140, L43.Google Scholar
Davis, M, Huchra, J, Latham, D W & Toury, J, 1982. Astrophys J 253, 423.Google Scholar
Krumm, N & Brosch, N, 1984. Astron J 89, 1461.Google Scholar