Does multiclustering of galaxy aggregates appear as a specific coil of extragalactic data unseparated from interpretations of the role of interstellar obscuration?

Details Does multiclustering of galaxy aggregates appear as a specific coil of extragalactic data unseparated from interpretations of the role of interstellar obscuration? Does multiclustering of galaxy aggregates appear as a specific coil of extragalactic data unseparated from interpretations of the role of interstellar obscuration?

Jan 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.129..403g&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 129, no. 2, Jan. 1987, p. 403-406.

Astronomy and Astrophysics

Astrophysics

2

Galactic Clusters, Galactic Evolution, Interstellar Extinction, Mass Distribution, Cosmic Dust, Cosmology, Galactic Structure, Star Distribution, Voids

Scientific paper

In the Jagiellonian Field (JF) the galaxies form themselves into a type of Pallium embedding the so-called Central Void. The popular suggestion was that the Jagiellonian Pallium/Patchy Structure (JPS) is caused by real existence of genuinely empty volume of interciuster space or - in terms of the Estonian School hypothesis - of intracellular space. Interstellar obscuration was never considered as an explanation of JPS, probably because of cosecant-type law which makes galactic extinction improbable; secondly, because of Zwicky and Rudnicki suggestions that the region of sky is free of selective extinction, and thirdly because of tradition (specific `problem-situation') in extragalactic astronomy that clusters of galaxies form real - not false - extended galaxy structures and multiclustering is not produced by dust obscuration. It is shown that a small and relatively dense cloud, at galactic latitude b = 720, of galactic dust contributing to the average extinction about 0'~O1 is projected just into the region of the Central Void. Interstellar obscuration affects multiclustering phenomenon in more serious degree than it can be theoretically predicted and/or reconstructed from studied distribution of stars. We confirm the view of Zi~ba that hierarchy of interstellar clouds of dust must lead to hierarchical clustering of galaxies

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