Table 4
Results on the extended emission.
| Fex [mJy] | Ffuv [mJy] | Res [AU] | tkin [yrs] | |
|---|---|---|---|---|
| U Ant | 1.3 | – | 50 000 | 23 700 |
| R Dor | 12.7 | – | 37 000 | 17 500 |
| β Gru | 9.7 | 3.83 | 58 000 | 27 500 |
| W Hya | 0.6 | – | 6 250 | 3 000 |
| TV Psc | 0.07 | 0.174 | 6 600 | 3 100 |
| RZ Sgr | 1.6(*) | – | 180 000 | 85 000 |
| DM Tuc | 1.1 | 3.53 × 10−3 | 10 000 | – |
| V420 Vul | 3.7 | – | – | – |
Notes. FUV flux densities (Fex), radius (Res), and kinematic age (tkin) of the extended structures presented in Sect. 3. Ffuv is the GALEX FUV flux of the stars (Bianchi et al. 2017). We assumed an expansion velocity of the outflow of 10 km s−1 for all objects.(*) The FUV flux density of RZ Sgr used here corresponds only to the inner, more pronounced, emission.
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