Left: histogram of Megeath et al. (2012) IR-excess (Class II) stars that lack Apogee RVs as a function of distance from the filamentary spine. Subsets within 0.2 and 0.05 pc are indicated. Right: H-band magnitude distribution of these three populations, with the whole population scaled down by a factor 7 for ease of comparison. Full population and 0.2 pc subsample are statistically indistinguishable, nor is there any obvious bias from the H< 12.5 Apogee selection in the 0.05 pc subsample.
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