Jul 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995aipc..336..429f&link_type=abstract
Dark matter. AIP Conference Proceedings, Volume 336, pp. 429-432 (1995).
Physics
5
Dark Matter, Galaxy Clusters
Scientific paper
The theory of the formation of large-scale structure in the universe through the action of gravitational instability imply the existence of substantial amounts of baryonic dark matter, of the order of 50% of the total baryon content in the universe, in the ``voids'' or under-dense regions seen in the large-scale distribution of galaxies. We discuss also the large-scale structure of dark matter expected in voids and the present and future possibilities for the observation of this baryonic dark matter in ``voids.''
Doroshkevich Andrei G.
Fong Richard
Turchaninov Victor I.
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