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Testing the universality of star formation - II. Comparing separation distributions of nearby star-forming regions and the field

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Figure

Table 1. A summary of the separation ranges and contrasts from each binarysurvey used.
Figure 2. The distribution of spectral types among the targets of the binarysurveys of Cha I (red) and CrA (blue).
Figure 4. The stellar MFs of our regions as a function of stellar density whenwe consider the same contrast cuts and stellar masses within the separationranges 19–774 au (top), 62–620 au (middle) and 19–100 au (bottom)
Fig. 5) shows no statistically significant differences. In the wider
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