Table A.1.
clus model parameters for the Centaurus core.
| Parameter | Value | Parameter | Value |
|---|---|---|---|
| n0, 1 | 65521 m−3 | c | 0.33 |
| rtc1 | 2.48 × 10−3r500 | A | 98 |
| β1 | 0.599 | B | 6.4 × 10−4r500 |
| n0, 2 | 22685 m−3 | C | 0.9 |
| rtc2 | 2.63 × 10−2r500 | D | 0.88 |
| β2 | 0.778 | E | 1.97 × 10−5r500 |
| Tc | 0.74 keV | F | 14r500 |
| Th | 6.75 keV | G | 5.2 × 10−2 |
| rto | 0.15r500 | r500 | 1.88 (1022 cm)(a) |
| μ | 2.36 | rout | 1 |
| rtc | 4.5 × 10−2r500 | rmin | 1 |
| a | 0.12 | rmax | 0.06(b) |
| b | 0.54 | av | 119 km s−1(c) |
Notes. (a) r500 = 610 kpc (3000 arcsec; Walker et al. 2013). (b) For a Resolve field of view radius of ∼90 arcsec divided by r500 = 3000 arcsec and rout = 1. (c) In the clus model, the velocity parameter describes the magnitude of micro-turbulence, which is equal to 
times the 1D velocity dispersion.
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