Voids in the Jagiellonian field

Details Voids in the Jagiellonian field Voids in the Jagiellonian field

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.115..369g&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 115, no. 2, Oct. 1985, p. 369-376.

Astronomy and Astrophysics

Astrophysics

5

Galactic Clusters, Intergalactic Media, Missing Mass (Astrophysics), Star Distribution, Cosmic Dust, Galactic Structure, Voids

Scientific paper

The exotic topology of apparent voids in galaxy distribution, and complex affairs related to the Jagiellonian Pallium-patchy Structure (JPS)-like phenomenon, have recently been analytically addressed under suspicions that the JPS phenomenon is due to dark (dust) matter. A modification of Kwast's (1974) method is presently used to recognize the distinctive characteristics of patches and pallia, leading to the detection of intergalactic, rather than interstellar, dust populations. The string of dust thereby noted is 100 times greater than Zwicky's (1957) value of 4 Mpc.

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