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Table 3:

Spatial information for the averaged vibrational transitions shown in Figs. 5 and 7, and the radii used to model the kinematics.
HD 97048 cont. v(2-1) v(3-2) v(4-3) $R_{\rm in, out}^{\rm model}$
SPP [AU] 0 $14.8^{\pm 0.9}$ $16.5^{\pm 2.7}$ - 11
FWHM [AU]a $21.2^{\pm 1.6}$ $\geq $23.8 $^{\pm 1.1}$ $\geq $ $23.0^{\pm 1.1}$ - 100
HD 100546          
SPP [AU] 0 $9.6^{\pm 0.5}$ $9.4^{\pm 0.5}$ $9.9^{\pm 1.5}$ 8
FWHM [AU] $10.0^{\pm 0.9}$ $\geq $ $13.7^{\pm 0.6}$ $\geq $ $13.1^{\pm 0.6}$ $\geq $ $11.5^{\pm 0.7}$ 100
a Note that this FWHM is a function of continuum + line emission, but that the SPP has been corrected for the continuum dilution, and thus is a direct function of the CO emission. All values are directly derived from the 2D spectrum, and not the maximum value resulting from an alignment of the slit with the semi-major axis.

Source LaTeX | All tables | In the text

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