Table 6
Non-thermal pressure of radio lobes in the three galaxy clusters assuming minimum energy.
| νlow = 10 MHz | γmin = 1 | ||||||
| Cluster | L150(W/Hz) | α | V (kpc3) | Bmin (μG) | Pnth (dyne/cm2) | Bmin (μG) | Pnth (dyne/cm2) |
|
|
|||||||
| RX J1852.1+571 | 1.8 × 1025 | 0.5 | 8.4 × 103 | 9.6 | 2.8 × 10-12 | 15.1 | 7.1 × 10-12 |
| A2276 | 2.6 × 1025 | 0.9 | 2.4 × 105 | 5.5 | 8.1 × 10-13 | 22.7 | 1.4 × 10-11 |
| ZwCl 1829.3+6912 | 7.6 × 1025 | 0.7 | 2.7 × 105 | 5.4 | 8.5 × 10-13 | 15.2 | 6.7 × 10-12 |
Notes. Columns 1 and 2: radio source luminosity at 150 MHz and spectral index, taken from Murgia et al. (2011); Cols. 5 and 6: minimum energy magnetic field and non-thermal pressure assuming νlow = 10 MHz and k = 1; Cols. 7 and 8: minimum energy magnetic field and non-thermal pressure assuming γmin = 1 and k = 1.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.