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Table 1
Globular cluster sample.
| NGC | Alt. Name | r in | r out | rin/rc | rin/rh | rout/rh | rout/rt | E(B − V) | [Fe/H] |
| arcmin | arcmin | ||||||||
|
|
|||||||||
| 2419 | 0.0 | 7.0 | 0.0 | 0.0 | 7.3 | 1.0 | 0.11 | –2.12 | |
| 5024 | M 53 | 1.0 | 7.0 | 2.8 | 0.9 | 6.3 | 0.3 | 0.02 | –1.99 |
| 5272 | M 3 | 0.0 | 10.0 | 0.0 | 0.0 | 8.9 | 0.3 | 0.01 | –1.57 |
| 5466 | 0.0 | 10.0 | 0.0 | 0.0 | 4.4 | 0.3 | 0.00 | –2.22 | |
| 5904 | M 5 | 0.0 | 10.0 | 0.0 | 0.0 | 4.7 | 0.3 | 0.03 | –1.34 |
| 6205 | M 13 | 1.0 | 10.0 | 1.3 | 0.7 | 6.7 | 0.4 | 0.02 | –1.54 |
| 6341 | M 92 | 0.0 | 10.0 | 0.0 | 0.0 | 9.2 | 0.7 | 0.02 | –2.28 |
| 7078 | M 15 | 0.0 | 10.0 | 0.0 | 0.0 | 9.4 | 0.5 | 0.10 | –2.32 |
| 7089 | M 2 | 1.0 | 10.0 | 2.9 | 1.1 | 10.7 | 0.5 | 0.06 | –1.62 |
Notes. Global parameters are from the most recent version of the Harris (1996) on-line database (year 2003), except for [Fe/H] for both M 5 and M 15, which are taken from Carretta et al. (2009a), and structural parameters for NGC 2419 that are taken from Bellazzini (2007).
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