Table 3
Some of the physical properties of the globular clusters studied in this work.
| Section | Cluster | RA | Dec | D⊙ | D gc | [Fe/H] | E(B−V) | V HB | V−MV | c | ρ 0 | FWHM | t exp |
| NGC | J2000 | J2000 | kpc | kpc | mag | mag | mag | log(L⊙ pc-3) | arcsec | s | |||
|
|
|||||||||||||
| 8.1 | 104 | 00:24:05.67 | −72:04:52.6 | 4.5 | 7.4 | −0.72 | 0.04 | 14.06 | 13.37 | 2.07 | 4.88 | 0.61 | 302.4 |
| 8.2 | 5139 | 13:26:47.24 | −47:28:46.5 | 5.2 | 6.4 | −1.53 | 0.12 | 14.51 | 13.94 | 1.31 | 3.15 | 0.38 | 312.0 |
| 8.3 | 5286 | 13:46:26.81 | −51:22:27.3 | 11.7 | 8.9 | −1.69 | 0.24 | 16.63 | 16.08 | 1.41 | 4.10 | 0.37 | 316.8 |
| 8.4 | 6093 | 16:17:02.41 | −22:58:33.9 | 10.0 | 3.8 | −1.75 | 0.18 | 16.10 | 15.56 | 1.68 | 4.79 | 0.45 | 302.4 |
| 8.5 | 6121 | 16:23:35.22 | −26:31:32.7 | 2.2 | 5.9 | −1.16 | 0.35 | 13.45 | 12.82 | 1.65 | 3.64 | 0.49 | 180.0 |
| 8.6 | 6541 | 18:08:02.36 | −43:42:53.6 | 7.5 | 2.1 | −1.81 | 0.14 | 15.35 | 14.82 | 1.86 | 4.65 | 0.56 | 340.8 |
| 8.7 | 6656 | 18:36:23.94 | −23:54:17.1 | 3.2 | 4.9 | −1.70 | 0.34 | 14.15 | 13.60 | 1.38 | 3.63 | 0.50 | 297.6 |
| 8.8 | 6681 | 18:43:12.76 | −32:17:31.6 | 9.0 | 2.2 | −1.62 | 0.07 | 15.55 | 14.99 | 2.50 | 5.82 | 0.49 | 312.0 |
| 8.9 | 6723 | 18:59:33.15 | −36:37:56.1 | 8.7 | 2.6 | −1.10 | 0.05 | 15.48 | 14.84 | 1.11 | 2.79 | 0.51 | 360.0 |
| 8.10 | 6752 | 19:10:52.11 | −59:59:04.4 | 4.0 | 5.2 | −1.54 | 0.04 | 13.70 | 13.13 | 2.50 | 5.04 | 0.59 | 198.0 |
Notes. Column 1 contains the section with the individual results for each globular cluster. Column 2 contains the name of the cluster as it is defined in the New General Catalogue, Cols. 3 and 4 contain the celestial coordinates (right ascension and declination), Col. 5 shows the distance from the Sun, Col. 6 is the distance from the Galactic centre, Col. 7 shows metallicity, Col. 8 shows reddening, Col. 9 shows V magnitude level of the horizontal branch, Col. 10 shos V distance modulus, Col. 11 shows King-model central concentration c = log (rt/rc), Col. 12 contains central luminosity density log 10(L⊙ pc-3), Col. 13 contains the mean FWHM (arcsec) measured in the reference image and Col. 14 shows the exposure time in the reference image.
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