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Corona Borealis Supercluster

Supercluster in the constellation Corona Borealis

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Observational history

Astronomers C. Donald Shane and Carl A. Wirtanen were the first to note a concentration or "cloud" of "extragalactic nebulae" in the region during a large-scale survey of extragalactic structures in the sky. George Abell was the first to note the presence of what he called "second-order clusters", namely clusters of clusters in the first publication of his Abell catalogue in 1958.

Postman and colleagues were the first to study the supercluster in detail in 1988, calculating it to have a mass of 8.2×1015 M☉, and contain the Abell clusters Abell 2019, Abell 2061, Abell 2065, Abell 2067, Abell 2079, Abell 2089, and Abell 2092. Abell 2124 lies 33 megaparsecs (110 million light-years) from the center of the supercluster and has been considered part of the group by some authors.

Abell 2069 lies close by but is more distant, with a line-of-sight association only.

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