Mass profiles of galaxy clusters from X-ray analysis
We review the methods adopted to reconstruct the mass profiles in X-ray luminous galaxy clusters. We discuss the limitations and the biases affecting these measurements and how these mass profiles can be used as cosmological proxies.
Gespeichert in:
| Hauptverfasser: | , , , , , , |
|---|---|
| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
16 April 2013
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| In: |
Space science reviews
Year: 2013, Jahrgang: 177, Pages: 119-154 |
| ISSN: | 1572-9672 |
| DOI: | 10.1007/s11214-013-9976-7 |
| Online-Zugang: | Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1007/s11214-013-9976-7 Verlag, lizenzpflichtig, Volltext: http://adsabs.harvard.edu/abs/2013SSRv..177..119E |
| Verfasserangaben: | Stefano Ettori, Annamaria Donnarumma, Etienne Pointecouteau, Thomas H. Reiprich, Stefania Giodini, Lorenzo Lovisari, Robert W. Schmidt |
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| 520 | |a We review the methods adopted to reconstruct the mass profiles in X-ray luminous galaxy clusters. We discuss the limitations and the biases affecting these measurements and how these mass profiles can be used as cosmological proxies. | ||
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