Open Access

Fig. 15.


Surface stellar density on the scale of UWPs (red dots), NESTs (light blue dots), loose groups (dark blue dots) as defined in Kirk & Myers (2011), the 3 main filaments as a whole and the whole Taurus cloud (black dots). This plot outlines two main free scale regimes, respectively associated to UWPs (red line) and the various structures on larger scales (blue line).

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