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Fig. 5

image

Ideal 12C12O (32) velocity-channel map of a T Tauri disk model with an embedded Jupiter-mass planet. The flux density in Jy/as2 is color coded for each individual channel. The inclination of the disk is 10° and the disk has a total mass of 2.67 × 10-5 M. The gap is visible but does not appear as a symmetric ring like in the continuum case because the parts of the disk contributing in the individual channel maps change due to Doppler shift.

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