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FM 22. Mapping the Frontier Fields with Chandra X-ray Observations

Published online by Cambridge University Press:  27 October 2016

C. Jones ,
R. van Weeren ,
G. Ogrean  and
W. Forman
C. Jones
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St. Cambridge, MA 02138, USA email: [email protected]
R. van Weeren
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St. Cambridge, MA 02138, USA email: [email protected]
G. Ogrean
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St. Cambridge, MA 02138, USA email: [email protected]
W. Forman
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St. Cambridge, MA 02138, USA email: [email protected]
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Abstract

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Chandra has deeply observed the clusters and parallel fields in four Frontier Fields. These observations allow us to dramatically improve our understanding of cluster mergers by comparing the detailed mapping of the hot cluster gas with high resolution mass maps and by identifying merger shocks and cold fronts. In merging clusters, relativistic particles can be re-accelerated to produce radio relics. A comparison of lensing maps and Chandra images allows us to determine the cluster morphology and dynamical state and if there are offsets between the dark matter and the hot gas.

Keywords

X-rays: galaxies: clustersdark matteracceleration of particlesgravitational lensinggalaxies:peculiar
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , General Assembly A29B: Astronomy in Focus , August 2015 , pp. 758 - 759
Copyright
Copyright © International Astronomical Union 2016 

References

Bonafede, A. et al. 2012, MNRAS, 426, 40 Google Scholar
Ebeling, et al. 2004, ApJ (Letters), 609, L49 Google Scholar
Ebeling, et al. 2007, ApJ (Letters), 611, L33 Google Scholar
Harvey, et al. 2015, Science, 347, 1462 Google Scholar
Jauzac, et al. 2012, MNRAS, 426, 3369 Google Scholar
Jauzac, et al. 2014, MNRAS, 443, 1549 Google Scholar
Mann, C. & Ebeling, H. 2012, MNRAS, 420, 2120 CrossRefGoogle Scholar
Ogrean, G. et al. 2015, ApJ, 812, 153 CrossRefGoogle Scholar
Owers, M., Randall, S., Nulsen, P., Couch, W., David, L., & Kempner, J. 2011, ApJ, 728, 27 Google Scholar
Owers, M., Couch, W., Nulsen, P., & Randall, S. 2012, ApJ (Letters), 750, L23 Google Scholar
van Weeren, et al. 2009, A&A, 505, 991 Google Scholar
van Weeren, et al. 2015, ApJ submittedGoogle Scholar
Zitrin, A. et al. 2009, ApJ (Letters), 707, L102 Google Scholar