Fitting of dust spectra with genetic algorithms - I. Perspectives and limitations

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Table 1:

Dust species used for fitting the ISO spectra with DUSTY.
f-Number	Species	Formula	Ref.
f₁	Amorphous aluminum oxide	Al₂O₃	1
f₂	astronomical silicate	SiO₄	2
f₃	Amorphous pyroxene (100K)	Mg_xFe_1-xSiO₃	3
f₄	Amorphous melilite	Ca₂Al₂SiO₇	4
f₅	Amorphous olivine	Mg_0.1Fe_1.2SiO₄	5,6
f₆	Crystalline magnesiowustite	Mg_0.1Fe_0.9O	7
f₇	Amorphous Mg-Fe-silicate	MgFeSiO₄	8
f₈	Crystalline spinel	MgAl₂O₄	9

References. (1) Begemann et al. (1997); (2) Ossenkopf et al. (1992); (3) Henning & Mutschke (1997); (4) Mutschke et al. (1998); (5) Jäger et al. (1994); (6) Dorschner et al. (1995); (7) Henning et al. (1995); (8) Hanner (1988); (9) Posch et al. (1999).

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