Figure 5.
Results of the cross-spectra analysis in the core of the Perseus Cluster shown in Fig. 4. Left: results from the entire central r ∼ 3.5 arcmin (∼70 kpc) region. Right: results from the selected dotted region (Fig. 4). Top row: amplitude of the volume emissivity fluctuations in the soft and hard bands, cross-amplitudes, measured coherence C and ratio R. Bottom row: the corresponding C and R maps. Notation and colour coding are the same as in Fig. 3. The ellipses show a range of parameters that lead to the observed values of C and R. The sizes of the ellipses reflect statistical and systematic uncertainties. Black ellipse: the entire r = 3.5 arcmin region, white ellipse: the selected dotted region (Fig. 4). The fluctuations in the central region are predominantly isobaric.

Results of the cross-spectra analysis in the core of the Perseus Cluster shown in Fig. 4. Left: results from the entire central r ∼ 3.5 arcmin (∼70 kpc) region. Right: results from the selected dotted region (Fig. 4). Top row: amplitude of the volume emissivity fluctuations in the soft and hard bands, cross-amplitudes, measured coherence C and ratio R. Bottom row: the corresponding C and R maps. Notation and colour coding are the same as in Fig. 3. The ellipses show a range of parameters that lead to the observed values of C and R. The sizes of the ellipses reflect statistical and systematic uncertainties. Black ellipse: the entire r = 3.5 arcmin region, white ellipse: the selected dotted region (Fig. 4). The fluctuations in the central region are predominantly isobaric.

Close
This Feature Is Available To Subscribers Only

Sign In or Create an Account

Close

This PDF is available to Subscribers Only

View Article Abstract & Purchase Options

For full access to this pdf, sign in to an existing account, or purchase an annual subscription.

Close