Interacting galaxies in the Hercules supercluster of galaxies. I - Ring galaxies

Astronomy and Astrophysics – Astronomy

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Celestial Mechanics, Galactic Clusters, Galactic Structure, Interacting Galaxies, Ring Galaxies, Astronomical Photography, H Ii Regions, Rings

Scientific paper

Four ring galaxies and two candidates have been discovered in the Hercules supercluster of galaxies by applying the photographic contrast-enhancement technique to deep IIIa-J or IIIa-F Schmidt plates. They appear to belong either to cluster halos or to a field population. IC 1194 has been found to have the largest linear diameter (≡133 kpc: on the scale of H0 = 55 km s-1Mpc-1) and the brightest magnitude (MV = -22.2) so far found. It shows no patchy structure on its ring, and hence no prominent H II regions. This is probably an S0-ring galaxy, i.e., a ring galaxy whose progenitor might have been a gas-free S0 galaxy. Dressler #36 of the Abell 2151 cluster has six bright knots which are surrounded by a faint diffuse ring. This is quite reminiscent of the structure of a self-gravitating ring undergoing "bead instability".

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