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Fig. 1

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Coordinate system of the starless core on the (x,z)-plane with the direction towards the observer. The position in the plane of the sky is defined by r0. Each line of sight, ŝ, corresponds to a distinct visual extinction, AV, calculated from the gas volume density profile along this direction. At a location ri on the sight line, the physical parameters (such as gas density, temperature, and radiation field) are assumed to be uniform on the dashed circle.

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