The dust condensation sequence in red supergiant stars

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Table 2:

Dust species used in this study with their commonly-used name, their size, shape and the source of the optical constants. The size distribution is that derived by Mathis et al. (1977) and the cross section are computed in the CDE (Continuous Distribution of Ellipsoids) approximation.
Name	Composition	Lattice structure	Size ( $N(\alpha)\sim\alpha^{-3.5}$ )	Shape	Reference
Alumina	Al₂O₃	amorphous	0.01-1 $\mu$ m	CDE	Begemann et al. (1997); Koike et al. (1995)
Melilite	Ca₂Al₂SiO₇	amorphous	0.01-1 $\mu$ m	CDE	Jaeger et al. (1994); Mutschke et al. (1998)
Olivine	Mg_0.8Fe_1.2SiO₄	amorphous	0.01-1 $\mu$ m	CDE	Dorschner et al. (1995)
MgFeO	Mg_0.1Fe_0.9O	amorphous	0.01-1 $\mu$ m	CDE	Henning et al. (1995)
Metallic iron	Fe	crystalline	0.01-1 $\mu$ m	CDE	Henning & Stognienko (1996)
Carbon	C	amorphous	0.01-1 $\mu$ m	CDE	Preibisch et al. (1993)

Source LaTeX | All tables | In the text

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