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Table 3.
AGN luminosity for the MaNGA sample of 13 dwarf galaxies.
| MaNGA | log(LOIII) | log(Lbol) | log[(dE/dt)/(Lbol)] |
|---|---|---|---|
| plateifu | (erg s−1) | (erg s−1) | |
| (1) | (2) | (3) | (4) |
| 10223–3702 | 40.5 | 43.5 | –5.4 |
| 10226–1901 | 39.8 | 42.8 | –6.4 |
| 11022–12702 | 37.4 | 40.4 | –4.8 |
| 11754–3701 | 40.2 | 43.2 | –6.7 |
| 11826–12702 | 37.4 | 40.4 | –4.7 |
| 12487–3704 | 40.3 | 43.3 | –6.6 |
| 7992–6102 | 39.8 | 42.8 | –6.6 |
| 8252–1902 | 39.2 | 42.2 | –4.9 |
| 8442–1901 | 40.0 | 43.0 | –4.6 |
| 8655–6101 | 38.8 | 41.8 | –5.4 |
| 8657–6104 | 36.9 | 39.9 | –4.5 |
| 8982–3703 | 41.3 | 44.3 | –4.8 |
| 9889–1902 | 40.9 | 43.9 | –5.2 |
Notes. (1) MaNGA plateifu; (2) [OIII] luminosity; (3) AGN bolometric luminosity derived as Lbol = 1000 × L[OIII] (Moran et al. 2014); (4) Ratio between the kinetic outflow rate of the outflow and the bolometric luminosity of the AGN.
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