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Table 6

Assumed submm/mm dust opacities, normalized to g2d = 100.

Opacity reference κ350 μm κ870 μm κ1.3 mm M a (κM)/(κ0M0) Note
(cm2 g-1) (cm2 g-1) (cm2 g-1) (M) 350,   870,   1300 μm

1D-models
This work (M0,κ0) 11.78 2.148 0.9621 5.5 1.0,   1.0,   1.0 T = 10−50 K, OH No. 22, β = 1.89
Johnstone et al. (2000) ··· 1.0 a,b ··· 8.1 (5.2) 0.7 (0.4) T = const. = 20 K (T = 13−42 K)
André et al. (2007) ··· ··· 0.5a 7.5 0.5 T = const. = 12 or =20 K
3D-models
Model Ic 2.87 0.406 0.1846 10.4 0.5,   0.4,   0.4 MgFeSi grains for amax = 3μm
Model II.1d 11.17 1.825 0.8206 7.3 1.3,   1.1,   1.1 Modified OH No. 22, i.e., β = 1.99
Model II.2e 2.05 0.376 0.1886 36.7 1.2,   1.2,   1.3 Mass for g2d = 100
Model II.3f 2.00 0.393 0.2073 36.2 1.1,   1.2,   1.4 RV = 5.5 and PAHs

Notes.

(a)

For the ρ Oph A core with assumed gas-to-dust mass ratio of g2d = 100.

(b)

Refers to 850 μm.

(d)

Modified Curve No. 22 of Ossenkopf & Henning (1994) using submm-β = 1.99, but normalized at 100 μm, i.e. β350−100 μm = 2.18.

(e)

M = 59.1 M: unmodified BARE-GR-S assumes g2d = 161 (Zubko et al. 2004).

(f)

M = 38.0 M: RV = 5.5 curve of Weingartner & Draine (2001) that includes PAHs assumes g2d = 105.1.

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