Transmission spectral properties of clouds for hot Jupiter exoplanets

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Table 3

Vibrational modes for the major diatomic bond species in the different cloud condensates considered in this paper.

Major	Reduced	Vibrational	Wavelength,
bond	mass, μ_M	frequency, ν	λ
	(g)	(cm^-1)	(μm)

Si−O	10.192	1110−830^a	9−12
Al−O	10.043	1100−350^c	9−28.7
Fe−O	12.436	790^b	12.5
Ti−O	11.99	850−150^d	16−66
MnS	20.247	295-220^e	20.2
ZnS	21.51	464^f	21.5
NaCl	13.95	366^g	13.95
KCl	18.60	281^g	18.6
C−H	0.923	3032^a	3.3

Notes.

^(a)

Glassgold & Graham (2008);

^(b)

Lehnert et al. (2002);

^(c)

Saniger (1995);

^(d)

Gillet et al. (1993);

^(e)

Batsanov & Derbeneva (1969);

^(f)

Kröger & Meyer (1954);

^(g)

Rice & Klemperer (2004).

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