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 . 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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