Comparison of fugitive and membership probabilities of members and fugitives. Stars close to the vertical line p_m = 0 are clearly not members, and those close to the main diagonal are not fugitives. Stars in between could be classified as members or fugitives depending on the value of p_min, but the number of such stars is very low. The only cluster where there are more than a handful of in-between stars is NGC 2516. This is due to the fact that it is the farthest away and, therefore, its stars have the most uncertain phase space coordinates. Even so, most of the ambiguous stars have low membership and fugitive probabilities.