Open Access

Table A.1

Ellipticity of GCs

Cluster ϵ ϵC10 ϵH10 ϵF14 Θ NPCA Photometric ΘF14 NF14 ΘM23 NM23
NGC 5139 0.064 ± 0.002 0.210 ± 0.020 0.17 0.671 147516
NGC 104 0.059 ± 0.004 0.160 ± 0.020 0.09 0.668 102838 0.064 28588
NGC 6752 0.023 ± 0.006 0.040 ± 0.020 0.04 0.417 38979 0.040 13721
NGC 6205 0.050 ± 0.007 0.120 ± 0.020 0.11 0.018 ± 0.011 0.416 28204 0.043 152392

Notes. The complete version of this table is available at the CDS. To estimate the ellipticity, we consistently applied the definition ϵ=1λb/λa=1b/a$ = 1 - \sqrt {{\lambda _b}/{\lambda _a}} = 1 - b/a$. The columns Θ, ΘF14, and ΘM23 represent the angular scale used to measure the ellipticities in their respective papers, measured in degrees. This scale is determined by measuring the angular separation in degrees between the cluster’s center and the most distant star in the sample. This column was not determined for the H10 and C10 samples as the data are not available. For the same reason, the θ14 column for NGC 6626 is left empty. The columns NPCA, NF14, and NM23 represent the number of stars in each sample.

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