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Rebusco, Paola (2007): Impact of supermassive black holes on galaxy clusters. Dissertation, LMU München: Fakultät für Physik

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Figure

Figure 1.1: Left: X-ray image of the Perseus cluster (XMM-Newton satellite,∼ 600 × 600 kpc, Churazov et al
Figure 1.3:X-ray spectrum of the Virgo galaxy cluster observed by thethe vertical axis represents the distribution of the number of photons at eachenergy
Figure 1.4: Ophiuchus cluster. Gas density radial profile from the EinsteinHRI and the ASCA data; the solid line is the best-fit β-model (Matsuzawa etal, 1996).
Figure 1.6:RGS spectra vs cooling flow models for a sample of massiveof emission lines from gas at the lowest temperatures (the lack of lines between13 and 18 clusters (Peterson et al
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