Primordial segregation in globular clusters: The degree of mass segregation as determined through dynamical models

Open Access

Fig. C.1

Half-mass radius normalized to tidal radius as function of mass for models with $Φ_{0} = 0.001 M_{⊙}^{- 1}$ $Mathematical equation: ${{\rm{\Phi }}_0} = 0.001{\rm{ M}}_ \odot ^{ - 1}$$ , α = −2.0 and m_max = 1.0 M_⊙ yielding $β = 2.36 \times 10^{- 2} M_{⊙}^{- 1}$ $Mathematical equation: $\beta = 2.36 \times {10^{ - 2}}{\rm{M}}_ \odot ^{ - 1}$$ (panel a), and with m_max = 100 M_⊙ giving $β = 7.99 \times 10^{- 5} M_{⊙}^{- 1}$ $Mathematical equation: $\beta = 7.99 \times {10^{ - 5}}{\rm{M}}_ \odot ^{ - 1}$$ (panel b).

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