Second-generation pancakes, and the formation of phantom galaxy clusters

Details Second-generation pancakes, and the formation of phantom galaxy clusters Second-generation pancakes, and the formation of phantom galaxy clusters

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983pazh....9..515d&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 9, Sept. 1983, p. 515-518) Soviet Astronomy Letters (ISSN 0360-0327), vol. 9, Sept.-Oct

Astronomy and Astrophysics

Astronomy

2

Cosmology, Galactic Clusters, Galactic Evolution, Interstellar Gas, Neutrinos, Photoionization, X Ray Astronomy

Scientific paper

The problem of formation of the second generation hot neutrino-gaseous "pancakes" is analyzed. These "pancakes" can evolve later into gravitationally bounded hot neutrino-gaseous clouds - "fantomes" of clusters. The temperature, mass and other parameters of "fantomes" are close to those of clusters of galaxies but "fantomes" do not (or nearly do not) contain ordinary galaxies. It is suggested that "fantomes" can be found in the X-ray surveys or by temperature fluctuations of relic radiation.

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