A search for H I in intercluster and cosmic void spaces

Details A search for H I in intercluster and cosmic void spaces A search for H I in intercluster and cosmic void spaces

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...344..597b&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 344, Sept. 15, 1989, p. 597-603.

Astronomy and Astrophysics

Astronomy

5

Galactic Clusters, H I Regions, H Lines, Hydrogen Clouds, Quasars, Dwarf Galaxies, Intergalactic Media, Radio Sources (Astronomy)

Scientific paper

A sample of radio-loud QSOs has been examined for the presence of narrow 21 cm H I lines originating in the redshift range from 3000 to 10,000 km/s with the Arecibo radio telescope. No probable or definite absorption or emission lines have been found, putting stringent limits on the volume density of small neutral hydrogen clouds or gas-rich dwarf galaxies, both in the void toward Perseus-Pisces and in the nearby superclusters.

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