Bottom-up dust nucleation theory in oxygen-rich evolved stars - I. Aluminium oxide clusters

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Table 9

Overview of recent observations of the species AlO, AlOH, and AlCl in the inner winds of oxygen-rich AGB stars of SRV and Mira types.

Species	SRV	MIRA	Reference
AlO	3.7(−8)	0	Decin et al. (2017)
	7.8(−8)	0	Danilovich et al. (2020)
		5.0(−10)	Kamiński et al. (2016)
	4.4(−8)	0	De Beck et al. (2017)
AlOH	6.9(−10)	2.1(−9)	Decin et al. (2017)
AlCl	9.2(−9)	4.1(−10)	Decin et al. (2017)

Notes. A conversion factor of ~0.46 is applied to some molecules to translate from relative (with respect to H₂) to fractional(with respect to the total gas including He) abundances. The fractional abundances (normalised to the total gas) are given as a(b) = a × 10^b.

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