The possible interpretation of the central void in the Jagellonian Field

Title:

The possible interpretation of the central void in the Jagellonian Field

Creator:

Grabińska, Teresa and Zabierowski, Mirosław

Identifier:

https://cdk.lib.cas.cz/client/handle/uuid:ab2cf453-f1c8-4424-923e-29fd60f20077
uuid:ab2cf453-f1c8-4424-923e-29fd60f20077

Subject:

astronomy, galaxies, and Jagellonian Field

Type:

model:article and TEXT

Format:

bez média and svazek

Description:

The problem of interpretation of the so-called Central Void /CV/ in the Jagiellonian Field /JF/ is consldered. The galaxies in JF are inclined to group around CV into a pallium-like configuration. The popular suggestion that CV may reflects a really existlng and genuinely empty volume of the inter-multicluster space has been verified. So far any interstellar cloud was nover regarded as a possiblo explanation because of: 1. the cosecant-type laws descrlbing interstellar extlnctlon in the Milky Way, whlch made the galactlc extlnction at b=72” improbable, 2. the claims of the Zwicky´s School that JF was free of the extlnction, 3. the traditlonal view that multlclustering was not caused by absorptive dusty clouds, i.e. that the extended galaxy structures were not only apparent. The results of our work concem the conceptual foundatlons of the researoh programme oontained in early works of Splawa-Neyman /superclustors of galaxies called "clouds"/ and recent searches of Batuski and Burns on a poasible 300 Mpc filament of clusters of galaxies in Perseus-Pegasus. In the paper It ia proved that a local dusty cloud Is projected just onto the region of the Central Void.

Language:

Czech

Rights:

http://creativecommons.org/publicdomain/mark/1.0/
policy:public

Coverage:

441-443

Source:

Publications of the Astronomical Institute of the Academy of Sciences of the Czech Republic | 1987 Volume:63-70 | Number:69

Harvested from:

CDK

Metadata only:

false