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Fig. 19

image

SB2 orbit of 06404608+0949173 in NGC 2264. Component A is represented by large circles and component B by small circles. Squares represent the single radial velocity obtained when only one peak is visible in the CCF; these are not used to calculate the orbital solution, due to their larger uncertainties. The error on radial velocities amounts to ± 0.25 km s-1. The horizontal dotted line is V0.

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