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Table 3.

Galaxies in the vicinity of NGC 253.

Name Type Vh VLG DTRGB MB TI ΘN253 R R3D

(km s−1) (km s−1) (Mpc) (mag) (deg) (kpc)
NGC 253 Sc 260.6 ± 5 (a) 294 3.70 ± 0.03 ( † ) −21.15
Do II dSph −6.6 3.2 1.3 86
LV J0055−2310 dIr 249.6 ± 5 (a) 288 3.62 ± 0.18 ( ‡ ) −9.81 2.2 2.7 175 191
Scl–MM–Dw1 dSph 3.94 ± 0.63 (♭) −9.54 1.8 1.1 71 251
NGC 247 Sd 153.0 ± 5 (a) 208 3.72 ± 0.03 ( † ) −18.56 1.6 4.5 293 294
Do IV dSph −7.1 2.2 3.6 233
ESO 540−032 Ir 227.7 ± 0.9 (b) 285 3.63 ± 0.05 ( † ) −11.45 1.4 5.4 349 354
Do III dSph −8.3 1.4 5.3 343
DDO 6 dIr 295.3 ± 5 (a) 347 3.44 ± 0.15 ( † ) −12.45 1.3 4.3 277 373
Sculptor SR dTr −10.26 1.2 4.0 257
KDG 2 dTr 223.5 ± 2.7 (b) 290 3.56 ± 0.07 ( † ) −11.49 1.0 7.2 463 478
Scl–MM–Dw2 dSph 3.12 ± 0.32 (♯) −11.03 0.7 0.8 53 582
Sc 22 dSph 4.29 ± 0.07 ( † ) −10.50 0.5 5.4 350 699
NGC 7793 Sd 223.8 ± 5 (a) 247 3.63 ± 0.14 ( † ) −18.34 0.2 13.1 842 838
PGC 704814 Ir 270 ± 89 (c) 299 3.66 ± 0.18 ( ‡ ) −11.61 2.1 12.4 798 795
ESO 349−031 dIr 220.3 ± 5 (a) 229 3.21 ± 0.06 ( † ) −11.87 0.2 12.6 802 901
DDO 226 dIr 362.1 ± 5 (a) 413 4.92 ± 0.29 ( † ) −13.63 −0.3 3.2 1243
UGCA 442 Sm 266.7 ± 5 (a) 299 4.37 ± 0.15 ( † ) −14.71 −0.3 15.5 1274
NGC 625 Sm 394.9 ± 5 (a) 324 4.02 ± 0.07 ( † ) −16.50 −0.3 18.9 1307
NGC 59 dEem 367.6 ± 5 (a) 438 4.90 ± 0.07 ( † ) −15.57 −0.4 8.3 1349
PGC 6430 Im 391.7 ± 5 (a) 306 4.57 ± 0.13 ( † ) −15.68 −0.7 21.7 1778

Notes. The columns contain: (1) galaxy name; (2) morphological type; (3) Vh – heliocentric velocity in km s−1 with its error; (4) VLG – radial velocity with respect to the LG centroid (Karachentsev & Makarov 1996); (5) DTRGB – TRGB–distance in Mpc with a corresponding error; (6) MBB-band absolute magnitude of the galaxy; (7) TI – ‘tidal index’ indicating the value of the tidal influence from the main disturber (Karachentsev & Makarov 1999; Karachentsev et al. 2013); (8) ΘN253 – projected separation from NGC 253 in degrees; (9) R – projected distance to NGC 253 in kpc; (10) R3D – spatial distance to NGC 253 in kpc.

References. (a)Westmeier et al. (2017), (b)Bouchard et al. (2005), (c)Colless et al. (2003), ( † )Jacobs et al. (2009), ( ‡ )Karachentsev et al. (2021), (♭)Sand et al. (2014), (♯)Toloba et al. (2016).

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