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Table 3

Parameters used in our population synthesis calculation (cf. Fig. 4).

Parameter

star formation rate constant
considered time interval 35 Myr
velocity distribution Gaussian distribution (Brott et al. 2011b)
(σ = 141   km s-1, μ = 100 km s-1)
velocity range 0–570 km s-1
mass distribution Salpeter (1955) IMF
mass range 5–30 M
stellar model grid LMC (Brott et al. 2011a)

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