Table 5: Upper limits on the CRp scaling parameter $X_{\rm CRp}$ inferred from radio brightness profiles of the radio mini-halo of Perseus cluster for different values of B₀, $\alpha _B$ , and $\alpha _{\rm p}$ .
Model $\alpha _{\rm p}$ $B_0~[\mu \mbox{G}]$ $\alpha _B$ $X_{\rm CRp}^{\rm isobaric}$ $X_{\rm CRp}^{\rm adiabatic}$

1 2.3 10 0.5 0.016 0.006

2 2.1 10 0.5 0.014 0.005

3 2.5 10 0.5 0.033 0.011

4 2.7 10 0.5 0.096 0.031

5 2.3 5 0.5 0.027 0.009

6 2.3 20 0.5 0.012 0.004

7 2.3 10 0.7 0.017 0.006

8 2.3 10 0.9 0.019 0.006

**Table 5:** Upper limits on the CRp scaling parameter $X_{\rm CRp}$ inferred from radio brightness profiles of the radio mini-halo of Perseus cluster for different values of B₀, $\alpha _B$ , and $\alpha _{\rm p}$ .
Model	$\alpha _{\rm p}$	$B_0~[\mu \mbox{G}]$	$\alpha _B$	$X_{\rm CRp}^{\rm isobaric}$	$X_{\rm CRp}^{\rm adiabatic}$
1	2.3	10	0.5	0.016	0.006
2	2.1	10	0.5	0.014	0.005
3	2.5	10	0.5	0.033	0.011
4	2.7	10	0.5	0.096	0.031
5	2.3	5	0.5	0.027	0.009
6	2.3	20	0.5	0.012	0.004
7	2.3	10	0.7	0.017	0.006
8	2.3	10	0.9	0.019	0.006

Source LaTeX | All tables | In the text