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Fig. 11


Mass-radius relation for the cores (black crosses) and the elongated structure (blue cross) in G35.20N. The vertical length of the crosses denotes the uncertainty in the mass (see Table 4), while the horizontal length denotes a 10% error in the radius of the core (Table 2). The red solid line indicate the criteria for massive star formation by Kauffmann & Pillai (2010), with the gray area corresponding to the low-mass star formation region.

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