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Fig. 6

image

Statistical properties of the APOGEE strings (see also Table A.1). The blue histograms denote the normalized frequencies for the 25 APOGEE strings identified outside the Orion Nebula Cluster with positions l ≥ 209.3 deg or l ≤ 208.7 deg. From left to right and from top to bottom: a) number of sources per string; b) fraction of young APOGEE objects (i.e., with Spitzer and/or XMM counterparts) per string; c) total length; d) mean distance to the nearest member of the string; e) maximum velocity difference within a string; f) internal velocity dispersion per string. The vertical red dashed lines indicate the mean value in each of the above distributions.

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