Fig. 1

Continuum-subtracted H2 image of the southern part of the observed region, displayed with logarithmic scales. The sources are marked according to the following: diamonds represent Class 0 stars from Bontemps et al. (2010), circles are Class I from Bontemps et al. (2010), and the square is a candidate Class 0 observed only in Spitzer 24 μm , the labels P2, P3, P4, P5, Y1, Y2, Y3, Y4, and Y5 are the names we used to refer to each source throughtout our work. For more on the outflows and driving sources, see Table 1. As dashed lines, we also show the polarization vectors (Sugitani et al. 2011).
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