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Fig. 7.

image

Left panel: stellar line-of-sight velocity obtained by fitting the spectral region around the CO band heads at 2.3 μm. Middle panel: rotating disk model fitted to the stellar LOSV. Right panel: residuals between observation and model. The dashed lines show the zero-velocity line and the line-of-nodes of the model and where they cross indicates the center of the continuum emission. Clipped regions are indicated in gray.

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