On the straight arc in Abell 2390

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Dark Matter, Galactic Clusters, Gravitational Lenses, Mass To Light Ratios, Red Shift, Arcs, Catastrophe Theory, Taylor Series, Visible Spectrum

Scientific paper

The long 'straight arc' observed in the cluster of galaxies Abell 2390 is investigated. The formation of straight arcs is considered analytically in terms of fold and cusp catastrophes and two singular sections of a cusp, the 'beak-to-beak' and 'lips' 'calamities'. It is shown that a single cusp always produces curved images, while straight images can be formed by fold catastrophes and these two types of calamities. These results are used to derive detailed models for the observed features. It is found to be possible to derive a fold model by introducing a sheetlike dark mass distribution. Beak-to-beak models must postulate either an unseen cluster to balance Abell 2390 or an unseen galaxy to offset the closest cluster galaxy. The latter model is more structurally stable and consistent with the optical and IR data.

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