Structure of Abell 1995 from optical and X-ray data: a galaxy cluster with an elongated radio halo

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Fig. 2

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Field of the cluster A1995 (direct sky view with north up) observed with the INT in the R_H-band. Cluster members are indicated by circles, while nonmember galaxies are shown by squares (see Table 1). Numbers highlight the IDs of notable galaxies as in Fig. 1.

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