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Fig. 9


Variation of P and θp of the sources against their distances from the center of the core in L1521F. The stars we observed are shown as filled circles and those from the Heiles (2000) catalogue, chosen within a circular region of 1° around L1521F, are shown as open triangles. The location of the peak emission in CO towards L1521F (Crapsi et al. 2004) is chosen as the core center.

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