Energy equipartition in globular clusters through the eyes of dynamical models

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Table 3

Results of the second fitting approach.

ID	α	$Φ_{0} (M_{⊙}^{- 1})$ ${\Phi _0}\left( {M_ \odot ^{ - 1}} \right)$	σ₀ (mas yr⁻¹)
NGC 104	0.0 ± 7.9	15.3 ± 1.2	0.690 ± 0.008
NGC 5139	0 ± 31	5.64 ± 0.57	0.749 ± 0.003
NGC 5904	−2 ± 26	14.2 ± 7.5	0.260 ± 0.043
NGC 6266	−2 ± 15	17.5 ± 4.3	0.556 ± 0.017
NGC 6341	0 ± 18	18.0 ± 5.9	0.244 ± 0.033
NGC 6397	0 ± 17	17.0 ± 1.4	0.511 ± 0.030
NGC 6656	0.0 ± 5.7	11.1 ± 3.1	0.719 ± 0.012
NGC 6752	−1.0 ± 8.6	14.4 ± 3.4	0.419 ± 0.021

Notes. Table columns: cluster ID and estimated values for α, Φ₀, and σ₀. We report the parameter values according to the two most significant digits of the associated uncertainty.

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