The flared inner disk of the Herbig Ae star AB Aurigae revealed by VLTI/MIDI in the N-band

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Table 2:

Derived characteristics of the resolved emission for simple geometric models.
Wavelength	8 $\mu$ m	10 $\mu$ m	12.5 $\mu$ m
FWHM^a [mas]	$28 \pm 2$	$38 \pm 4$	$49 \pm 4$
[AU]	$4.6 \pm 0.3$	$5.5 \pm 0.6$	$7.1 \pm 0.6$
$F_{\rm gauss} / F_{\rm tot}$	$0.82 \pm 0.02$	$0.97 \pm 0.02$	$0.89 \pm 0.02$
FWHM^b [mas]	$19 \pm 5$	$36 \pm 4$	$43 \pm 8$
[AU]	$2.7 \pm 0.6$	$5.2 \pm 0.6$	$6.2 \pm 1.2$

^a Gaussian and unresolved emissions (lower limit of FWHM size).
^b Pure Gaussian emission (lower limit of FWHM size).

Source LaTeX | All tables | In the text

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