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An XMM-Newton observation of A3921: an off-axis merger by Belsole, E.; Sauvageot, J-L.; Pratt, G. W.; Bourdin, H. is a scholarly article available to read on EtoBox.
What is An XMM-Newton observation of A3921: an off-axis merger about?
We present the results of a detailed analysis of the XMM-Newton observation of the galaxy cluster Abell 3921. The X-ray morphology of the cluster is elliptical, with the centroid offset from the brightest cluster galaxy by 17 arcsec, and with a pronounced extension toward the NW. Subtraction of a 2D beta model fit to the main cluster emission reveals a large scale, irregular residual structure in the direction of the extension, containing both diffuse emission from the intra cluster medium, and extended emission from the second and third-brightest cluster galaxies (BG2 and BG3). The greatest concentration of galaxies in the subcluster lies at the extreme northern edge of the residual. The cluster exhibits a remarkable temperature structure, in particular a bar of significantly hotter gas, oriented SE-NW and stretching from the centre of the cluster towards BG2 and BG3. Our detailed study of the morphological and thermal structure points to an off-axis merger between a main cluster and a less massive galaxy cluster infalling from the SE. From comparison of the temperature map with numerical simulations, and with independent calculations based on simple physical assumptions, we concl
- Author
- Belsole, E.; Sauvageot, J-L.; Pratt, G. W.; Bourdin, H.
- Published
- 2004
- Language
- EN