Relation between the geometric shape and rotation of Galactic globular clusters

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Table A.2

Comparison of the median axial ratio from this paper with the literature values.

b/a from this paper	b/a from the literature	Reference	Number of clusters
${0.951}_{- 0.036}^{+ 0.021}$ $0.951_{ - 0.036}^{ + 0.021}$	${0.940}_{- 0.090}^{+ 0.050}$ $0.940_{ - 0.090}^{ + 0.050}$	H10	100
${0.948}_{- 0.046}^{+ 0.022}$ $0.948_{ - 0.046}^{ + 0.022}$	${0.865}_{- 0.095}^{+ 0.065}$ $0.865_{ - 0.095}^{ + 0.065}$	C10	116
${0.964}_{- 0.017}^{+ 0.011}$ $0.964_{ - 0.017}^{ + 0.011}$	${0.986}_{- 0.004}^{+ 0.009}$ $0.986_{ - 0.004}^{ + 0.009}$	F14	11
${0.935}_{- 0.090}^{+ 0.033}$ $0.935_{ - 0.090}^{ + 0.033}$			163

Notes. Median value, 16th and 84th percentiles of the distribution of b/a.

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