Table 22
Integrated V − I colours, dereddened V − I integrated colours, and age estimates of the globular clusters in which the X ray sources are located.
| Name | Class* | Age+ | V mag | VI | VI0 | Age† |
|
|
||||||
| B005 | confirmed | old | 15.69 | 1.29 | 1.15 | old |
| SK055B | candidate | – | 18.991 | 0.388 | 0.248 | – |
| B024 | confirmed | old | 16.8 | 1.15 | 1.01 | old |
| SK100C | candidate | na | 18.218 | 1.181 | 1.041 | old |
| B045 | confirmed | old | 15.78 | 1.27 | 1.13 | old |
| B050 | confirmed | old | 16.84 | 1.18 | 1.04 | old |
| B055 | confirmed | old | 16.67 | 1.68 | 1.54 | old |
| B058 | confirmed | old:: | 14.97 | 1.1 | 0.96 | old-inter |
| MITA140 | confirmed | old | 17 | 9999 | – | – |
| B078 | confirmed | old | 17.42 | 1.62 | 1.48 | old |
| B082 | confirmed | old | 15.54 | 1.91 | 1.77 | old |
| B086 | confirmed | old | 15.18 | 1.26 | 1.12 | old |
| SK050A | confirmed | – | 18.04 | 1.079 | 0.939 | old-inter |
| B094 | confirmed | old | 15.55 | 1.26 | 1.12 | old |
| B096 | confirmed | old | 16.61 | 1.48 | 1.34 | old |
| B098 | confirmed | old | 16.21 | 1.13 | 0.99 | old-inter |
| B107 | confirmed | old | 15.94 | 1.28 | 1.14 | old |
| B110 | confirmed | old | 15.28 | 1.28 | 1.14 | old |
| B117 | confirmed | old:: | 16.34 | 1 | 0.86 | inter |
| B116 | confirmed | old | 16.79 | 1.86 | 1.72 | old |
| B123 | confirmed | old | 17.416 | 1.29 | 1.15 | old |
| B124 | confirmed | old | 14.777 | 1.147 | 1.007 | old |
| B128 | confirmed | old:: | 16.88 | 1.12 | 0.98 | old-inter |
| B135 | confirmed | old | 16.04 | 1.22 | 1.08 | old |
| B143 | confirmed | old | 16 | 1.22 | 1.08 | old |
| B144 | confirmed | old:: | 15.88 | 0.59 | 0.45 | young |
| B091D | confirmed | old | 15.44 | 9999 | – | – |
| B146 | confirmed | old:: | 16.95 | 1.09 | 0.95 | interm |
| B147 | confirmed | old | 15.8 | 1.27 | 1.13 | old |
| B148 | confirmed | old | 16.05 | 1.17 | 1.03 | old |
| B150 | confirmed | old | 16.8 | 1.28 | 1.14 | old |
| B153 | confirmed | old | 16.24 | 1.3 | 1.16 | old |
| B158 | confirmed | old | 14.7 | 1.15 | 1.01 | old |
| B159 | confirmed | old | 17.2 | 1.41 | 1.27 | old |
| B161 | confirmed | old | 16.33 | 1.1 | 0.96 | old-inter |
| B182 | confirmed | old | 15.43 | 1.29 | 1.15 | old |
| B185 | confirmed | old | 15.54 | 1.18 | 1.04 | old |
| B193 | confirmed | old | 15.33 | 1.28 | 1.14 | old |
| SK132C | candidate | - | 18.342 | 1.84 | 1.7 | old |
| B204 | confirmed | old | 15.75 | 1.17 | 1.03 | old |
| B225 | confirmed | old | 14.15 | 1.39 | 1.25 | old |
| B375 | confirmed | old | 17.61:: | 1.02 | 0.88 | interm |
| B386 | confirmed | old | 15.547 | 1.154 | 1.014 | old |
Notes.
Classification as confirmed or otherwise comes from the revised Bologna catalogue (December 2009, Version 4) http://www.bo.astro.it/M31/RBC_Phot07_V4.tab.
age comes from Caldwell et al. (2009). V, and V − I are integrated colours that come from the revised Bologna catalogue (December 2009, Version 4) http://www.bo.astro.it/M31/RBC_Phot07_V4.tab, (V − I)0 is the dereddened V − I integrated colour, assuming E(B − V) = 0.10 ± 0.03, which is the average of the reddenings of all M 31 clusters in Rich et al. (2005). (this E(B − V) corresponds to E(V − I) = 0.14).
This dereddened colour (V − I)0 is used to estimate the age on the basis of the plots (V − I)0 versus log Age from Sarajedini et al. (2007).
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