Fig. 3
The visibilities and closure phases of HD 327083 as a function of spatial frequency. The closure phase measurements have been re-binned by a factor of 5. Closure phases observed with the UT1-UT2-UT3 configuration at spatial frequencies below 190 cycles per arcsecond have been omitted as these exhibited a large scatter. The solid lines represent the best fitting model discussed in Sect. 3.1.1.
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