Table 3.
LeMMINGs optical and radio properties.
| Galaxies | Number | Undetected | Core-Sérsic | |
|---|---|---|---|---|
| (ours/full sample) | (ours/full sample) | (our sample) | ||
| (1) | (2) | (3) | (4) | |
| E | 23 (13.2%)/26(9.3%) | 52.2%/50.0% | 65.2% | |
| S0 | 42 (24.3%)/55(19.6%) | 40.5%/41.8% | 11.9% | |
| S | 102 (59.0%)/189(67.1%) | 54.0%/60.3% | 0% | |
| Irr | 6 (3.5%)/10(3.6%) | 66.7%/70.0% | 0% | |
| Seyfert | 10 (5.8%)/18 (6.4%) | 20.0%/27.8% | 0% | |
| ALG | 23 (13.3%)/28 (10.0%) | 78.3%/75.0% | 34.5% | |
| LINER | 71 (41%)/94 (33.6%) | 30.1%/38.3% | 15.5% | |
| H II | 69 (39.9%)/140 (50.0%) | 67.6%/66.4% | 1.7% | |
| Total | 173 (100%)/280 (100%) | 52.0%/56.1% | 20/173(11.6%) | |
Notes. The sample galaxies are first separated based on the galaxy morphological and optical spectral classes (Cols. 1–2) and then further divided based on their radio non-detection and core-Sérsic type central structure (Cols. 3–4). The term ‘full sample’ refers to the total LeMMINGs sample of 280 galaxies, whereas the term ‘our sample’ refers to the sub-sample of 173 LeMMINGs galaxies studied in this paper.
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