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Table 6:

Gaussian FWHM of the different objects and emission components studied here (still convolved).
Band FWHM [ $^{\prime \prime }$/AU] Spectroscopy/
  target std. imaging
IRAS 06084-0611 (VLA1), TIMMI2
average 4.7/4900 - spectroscopy
@ 10.0 $\mu $m 2.8/2900 1.3/1400 spectroscopy
@ 11.2 $\mu $m 2.8/2900 1.1/1200 spectroscopy
@ 11.9 $\mu $m 2.9/3000 0.58/610 imaging
IRAS 06084-0611 (VLA4), TIMMI2
average 3.6/3800 - spectroscopy
@ 10.0 $\mu $m 1.2/1300 1.1/1200 spectroscopy
@ 11.2 $\mu $m 2.2/2300 1.3/1400 spectroscopy
@ 11.9 $\mu $m 2.0/2100 0.58/610 imaging
CD-42 11721 (star), TIMMI2
average 1.8/720 - spectroscopy
@ 11.9 $\mu $m 0.94/380 0.58/230 imaging (all frames)
@ 11.9 $\mu $m 0.78/300 0.58/230 imaging (shifted)
CD-42 11721 (patch+arc), TIMMI2
average 4.7/1900 - spectroscopy
TY Cra (PAH)
@ 10.0 $\mu $m 3.0/390 0.3/39 spectroscopy
@ 11.2 $\mu $m 3.5/460 0.3/39 spectroscopy
TY Cra (Dust/continuum), VISIR
@ 10.0 $\mu $m 1.0/130 0.3/39 spectroscopy
@ 11.2 $\mu $m 1.4/180 0.3/39 spectroscopy
HD 176386, VISIR
8-13 $\mu $m $\le$0.3/39 0.3/39 spectroscopy
K-band 0.52/68 - imaging

Source LaTeX | All tables | In the text

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