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Fig. 7


Frequency of strings detected in our Random (upper panel), Cauchy (middle panel), and Swapping (lower panel) models as functions of the number of members per string (Nmembers). The different shaded areas enclose the 1σ, 2σ, and 3σ dispersion in each of these models. In all panels, the blue squares represent the detected APOGEE strings in Orion A at l ≥ 210 deg. The vertical dashed line indicates the minimum number of sources considered to define our APOGEE strings, with Nmember ≥ 4.

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