High-redshift objects as probes of nearby cosmic voids

Details High-redshift objects as probes of nearby cosmic voids High-redshift objects as probes of nearby cosmic voids

Feb 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap%26ss..90..457b&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 90, no. 2, Feb. 1983, p. 457-460.

Physics

6

Absorption Spectra, Bl Lacertae Objects, Cosmic Gases, Cosmology, Matter (Physics), Quasars, Line Spectra, Red Shift, Spatial Distribution

Scientific paper

It is shown that present day observational techniques make it possible to detect diffuse gas masses down to approximately 10 to the 10th solar masses in cosmic voids with linear sizes of approximately 1 Mpc or larger. The observations consist of searches for absorption lines, similar in character to those produced in galactic interstellar clouds, in the spectra of high-redshift objects located beyond previously identified voids adjoining nearby superclusters.

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