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Table 4

Fit results of the spectral decomposition of the detected forsterite bands.

Relative mass fractions M.A.T Distance
Star at 50 K at 100 K at 150 K at 200 K at 295 K [K] AU

HD 100546 0.00 0.11 0.22 0.63 0.04 166–204 24–36
IRS 48 0.00 0.00 0.45 0.55 0.00 156–189 19–27
HD 144668 0.00 0.00 0.93 0.07 0.00 135–183 37–69
HD 179218 0.00 0.00 0.32 0.68 0.00 174–186 90– 103
HD 141569 0.00 0.00 0.37 0.23 0.40 148–248 13–38
HD 104237 0.00 0.00 0.00 1.00 0.00 180–211 23–32

at 8.K at 20.K at 50.K at 100.K at 150.K

AS 205 0.00 0.78 0.22 0.00 0.00 ~30 ~516

at 50 K, 3% Fe at 50 K, 4% Fe at 100 K, 3% Fe at 100 K, 4% Fe at 200 K, 3% Fe

AB Aur 0.75 0.00 0.10 0.15 0.00 ~63 ~304

Notes.Listed are the relative mass fractions of the forsterite components at different temperature or with different iron mass fractions. Also listed is the confidence intervals for the mass-average-temperature (M.A.T.) of the fitted dust components. The distance intervals are computed based on the ranges of dust temperature (see text).

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