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Fig. 5
Panel a: P-V diagram of IRAS 16342−3814 obtained from SHAPE model. Panel b: P-V diagram of IRAS 16342−3814 from ALMA observations. The faint emission in the upper right corner is due to the H13CO(J = 4 → 3) line. Both P-V diagrams were obtained using a slit along PA = 67°.
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