Table 1.
General properties of the galaxies in our sample.
| Galaxy | Morphological | Environment | Ref. | AGN | Ref. | DL | Scale | LX (2−10 keV) | Ref. |
|---|---|---|---|---|---|---|---|---|---|
| type | type | (Mpc) | (pc/″) | (erg s−1) | |||||
| Mrk 1066 | (R)SB0+(s) | Minor merger | 1,2 | Sy 2 | 5 | 47.2 | 224 | 7.8 × 1042 | 11 |
| NGC 2273 | SB(r)a | Isolated | 3 | Sy 2 | 6 | 25.8 | 124 | 1.9 × 1042 | 12 |
| NGC 4253 | (R’)SB(s)a | Isolated | 3 | Sy 1.5 | 7,8 | 57.8 | 272 | 5.5 × 1042 | 13 |
| NGC 4388 | SA(s)b | Virgo Cluster | 3 | Sy 1.9 | 9 | 19.4 | 93 | 3.2 × 1042 | 13 |
| NGC 7465 | (R’)SB(s)00 | NGC 7448 Group | 4 | Sy 2/L | 10 | 21.9 | 105 | 5.6 × 1041 | 13 |
References. Morphological types, distances, and scales are from NED. The last two are computed in the cosmic microwave background frame. Environment: (1) Gimeno et al. (2004), (2) Smirnova et al. (2010), (3) NED, (4) Van Driel et al. (1992). AGN types: (5) Goodrich & Osterbrock (1983), (6) Contini et al. (1998), (7) Osterbrock & Pogge (1985), (8) Osterbrock & Martel (1993), (9) Mason et al. (2015), (10) Ferruit et al. (2000). Spectral types are further discussed in the text. Intrinsic (absorption-corrected) X-ray luminosities in the 2–10 keV band: (11) Marinucci et al. (2012), (12) Awaki et al. (2009), (13) Ricci et al. (2017).
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