Abstract
Based on optical data we propose a dynamycal model for A115. From spatial and radial velocity distributions we find three massive subsclusters that configure a pre-merging scenario. On this basis, we discuss on the origin of the radio emission and its correlation with X-rays.
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Barrena, R., Boschin, W., Girardi, M. (2007). The Internal Dynamics of A115 Nearby Cluster of Galaxies. In: Saviane, I., Ivanov, V.D., Borissova, J. (eds) Groups of Galaxies in the Nearby Universe. ESO ASTROPHYSICS SYMPOSIA. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-71173-5_63
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DOI: https://doi.org/10.1007/978-3-540-71173-5_63
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-71172-8
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