A connection between the Perseus-Pisces supercluster and the A 569 cloud?

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Galactic Clusters, Galactic Structure, Hydrogen Clouds, Radio Galaxies, Red Shift, H I Regions, Line Spectra, Milky Way Galaxy

Scientific paper

In order to shed some light on the possibility of a connection between the Perseus-Pisces supercluster and the A 569 cluster through the zone of avoidance of the Galaxy, H I and optical observations of galaxies have been carried out in the region. Forty-two redshifts have been measured, among which 21 for the first time in the possible connection zone. The study of the H I contents of the galaxies detected in the 21-cm line shows they are perfectly normal; as a by-product of this study, the UGC magnitudes are found to be high by more than one magnitude for m/(UGC) greater than or equal to 17.

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