Table 1
The sample of nearby edge-on galaxies as targets of dedicated searches for associated dwarf galaxies.
Name | α J2000 | δ J2000 | l II | b II | V | D | log LB | Bulge |
(km s-1) | (Mpc) | (L⊙) | ||||||
|
||||||||
NGC 7814 | 00 03 14.89 | +16 08 43.5 | 106.4 | –45.2 | 1050 | 16 ± 3 | 10.2 | p + |
NGC 100 | 00 24 02.98 | +16 29 13.6 | 113.5 | –45.9 | 850 | 17 ± 3 | 9.1 | – |
UGC 1281 | 01 49 31.61 | +32 35 19.5 | 136.9 | –28.7 | 150 | 6 ± 1 | 8.6 | – |
ESO 477–G016 | 01 56 15.99 | –22 54 04.0 | 200.4 | –74.7 | 1825 | 36 ± 5 | 10.1 | m |
NGC 891 | 02 22 33.41 | +42 20 56.9 | 140.4 | –17.4 | 525 | 10 ± 1 | 10.4 | m + |
NGC 1886 | 05 21 48.15 | –23 48 36.5 | 226.3 | –29.6 | 1750 | 31 ± 5 | 9.8 | m + |
ESO 121–G006 | 06 07 29.86 | –61 48 27.3 | 271.0 | –28.8 | 1200 | 20 ± 3 | 9.5 | s |
NGC 2549 | 08 18 58.35 | +57 48 11.0 | 159.7 | +34.2 | 1075 | 17 ± 7 | 9.8 | p |
NGC 2654 | 08 49 11.83 | +60 13 16.2 | 156.1 | +37.8 | 1350 | 28 ± 4 | 10.0 | m |
UGC 5245 | 09 47 34.49 | –02 01 57.1 | 238.8 | +37.0 | 1400 | 21 ± 4 | 9.0 | – |
NGC 3098 | 10 02 16.69 | +24 42 39.9 | 206.8 | +52.1 | 1400 | 20 ± 6 | 9.7 | m |
NGC 3115 | 10 05 13.98 | –07 43 06.9 | 247.8 | +30.8 | 675 | 10 ± 2 | 10.3 | p |
UGC 5459 | 10 08 10.07 | +53 05 00.5 | 160.8 | +50.3 | 1100 | 22 ± 4 | 10.1 | – + |
NGC 3669 | 11 25 26.81 | +57 43 16.2 | 143.3 | +55.9 | 1940 | 43 ± 23 | 10.2 | s |
UGC 6792 | 11 49 23.30 | +39 46 17.4 | 164.5 | +72.0 | 850 | 20 ± 3 | 9.0 | – |
NGC 4179 | 12 12 52.11 | +01 17 58.9 | 281.6 | +62.6 | 1250 | 18 ± 4 | 9.9 | m |
UGC 7321 | 12 17 34.00 | +22 32 24.5 | 241.9 | +81.1 | 400 | 18 ± 6 | 9.1 | – |
NGC 4244 | 12 17 29.66 | +37 48 25.6 | 154.6 | +77.2 | 250 | 04 ± 2 | 9.7 | s + |
UGC 7394 | 12 20 27.66 | +01 28 11.1 | 285.5 | +63.3 | 1600 | 32 ± 3 | 9.2 | – |
NGC 4565 | 12 36 20.78 | +25 59 15.6 | 230.8 | +86.4 | 1225 | 12 ± 4 | 10.8 | m + |
ESO 575–G061 | 13 08 15.60 | –21 00 08.0 | 308.2 | +41.7 | 1650 | 29 ± 5 | 9.4 | – |
NGC 5170 | 13 29 48.79 | –17 57 59.1 | 315.7 | +44.0 | 1500 | 27 ± 7 | 10.9 | s |
UGC 8880 | 13 57 11.48 | +50 26 08.6 | 99.1 | +63.5 | 1850 | m | ||
NGC 5470 | 14 06 31.70 | +06 01 41.0 | 346.5 | +62.4 | 1025 | 24 ± 3 | 9.2 | m + |
UGC 9242 | 14 25 21.02 | +39 32 22.5 | 71.4 | +66.9 | 1475 | 20 ± 6 | 9.0 | – |
UGC 9249 | 14 26 59.78 | +08 41 01.0 | 358.2 | +60.9 | 1375 | 19 ± 3 | 8.9 | – |
NGC 5746 | 14 44 55.92 | +01 57 18.0 | 355.0 | +53.0 | 1725 | 30 ± 3 | 11.1 | m + |
NGC 5866 | 15 06 29.50 | +55 45 47.6 | 92.0 | +52.5 | 750 | 12 ± 4 | 10.1 | p + |
NGC 5907 | 15 15 53.77 | +56 19 43.6 | 91.6 | +51.1 | 675 | 16 ± 2 | 10.8 | – + |
UGC 9977 | 15 41 59.54 | +00 42 46.1 | 7.3 | +41.3 | 1925 | 29 ± 3 | 10.3 | – + |
ESO 146–G014 | 22 13 00.43 | –62 04 03.4 | 328.6 | –46.4 | 1700 | 21 ± 2 | 9.4 | – |
IC 5176 | 22 14 55.93 | –66 50 57.9 | 323.0 | –43.7 | 1750 | 27 ± 3 | 10.3 | s |
Notes. Column (1): source name. Columns (2)–(5): equatorial and Galactic coordinates. Column (6): systemic velocity from NED, rounded to 25 km s-1. Column (7): here and elsewhere in the text, distances D are average values from the literature given by NED. If there is no distance determination independent of radial velocity, no value is given. Column (8): the logarithm of the blue luminosity (LB in solar units) was taken from the “RC3” of de Vaucouleurs et al. (1991), correcting for inclination, internal extinction, and redshift. Only for NGC 1886, ESO 121–G006, and ESO 311–G012 were luminosities calculated from RC3 uncorrected blue magnitudes. Column (9): – indicates the apparent absence of a bulge; otherwise, with increasing dominance of a bulge, small = s, moderate = m, and prominent = p (see Sect. 4). A “+” indicates that at least some traces of an equatorial dust lane are present.
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