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Fig. 8

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Predicted emission maps for toy models (black contours) convolved by a Gaussian of FWHM, superimposed on the observed deconvolved H2 1–0 S(1) map from Fig. 1 (red contours). Top: hollow cone viewed 40° from pole-on with radius 60 AU and semi-opening angle 27°. Bottom: hollow half-sphere viewed 45° from pole-on, with radius 28 AU and center projected at 40 AU along the blue jet. All contours increase by factors of . The PSF of the spectrum at (0, 0) was subtracted in all cases.

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