1981The Astrophysical JournalRequires access

Observations of the two components of the Abell 98 cluster of galaxies

Joseph P. Henry, M. J. Henriksen, P. A. Charles, John R.  Thorstensen

Open publisher page 22 citations

Abstract

X-ray and optical observations of A98 show that the cluster is composed of two subclusters. From an estimate of the mass and velocity differences, the two components may merge in about a billion years. These data support the hierarchical clustering model in which clusters occur on all size scales, with larger clusters being formed from mergers of smaller ones.

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What this paper is about

X-ray and optical observations of A98 show that the cluster is composed of two subclusters. From an estimate of the mass and velocity differences, the two components may merge in about a billion years. These data support the hierarchical clustering model in which clusters occur on all size scales, with larger clusters being formed from mergers of smaller ones.

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Available abstract

X-ray and optical observations of A98 show that the cluster is composed of two subclusters. From an estimate of the mass and velocity differences, the two components may merge in about a billion years. These data support the hierarchical clustering model in which clusters occur on all size scales, with larger clusters being formed from mergers of smaller ones.

Key concepts: Physics, Abell 2744, Astrophysics, Brightest cluster galaxy, Galaxy cluster, Astronomy, Cluster (spacecraft), Galaxy groups and clusters

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