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Table 5

Physical properties of the star formation, assuming empirical relations and simple physical assumptions for an isolated starburst (Cols. 26, see also Sect. 5.2).

Empirical properties from SED Visual association of from images
Radio galaxy r SB t dyn sSFR ΣSFR ex situ (>5 kpc) in situ (<5 kpc) AGN-driven
[%] [kpc] [Myr] [Gyr-1] [M yr-1 kpc-2] likelihood

3C 368 6 2.7 22 44 12.0 low high medium
3C 470 2 2.4 21 46 12.8 medium? medium? none
MRC 0324-228 56 5.4 31 31 8.5 ... ... ...
PKS 1138-262 2 6.8 35 27 7.6 high low none
MRC 0406-244 61 7.7 37 26 7.2 none high low
MRC 2104-242 28 4.8 30 33 9.0 high medium? low?
USS 0828+193 6 3.4 25 39 10.7 none high medium?
4C 28.58 14 6.1 33 29 8.1 medium? medium? medium?
USS 0943-242 56 12.1 47 20 5.7 high low none
4C 41.17 (all) 44 12.1 47 20 5.7 high low medium
TN J2007-1316 11 6.1 33 29 8.1 high ... ...

4C 41.17 (compact) ... 1 2.5 400 3200 ... ... ...

Notes. All calculated values only take into account the SB component (see Sect. 5.2 for details). None of the indicated properties are fully constrained (except for 4C 41.17 (compact) where we constrain the size; see Sect. 5.3.3 for details). Columns 79 refer to the likelihood from visual inspection on images described in Sect. 5.3. Question marks refer to ambiguous case (see respective figures). (...) indicates a lack of data to assess any visual association.

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