The thermal emission of Centaurs and trans-Neptunian objects at millimeter wavelengths from ALMA observations

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Table 3

Additional thermal modeling fit results: Chariklo.

Object	Model	Diameter or	Geometric	Beaming	Thermal	Ref. for	Relative submm
		a, b, c (km)	albedo	factor	inertia (MKS)	submm/mm data	emissivity

Chariklo	TPM^a, no rough.	240	0.037	N/A	2.6	This work	1.24 (1.29 mm)

Chariklo	TPM^a, small rough.	240	0.037	N/A	4.3	This work	1.23 (1.29 mm)

Chariklo	TPM^a, interm. rough.	240	0.037	N/A	5.9	This work	1.22 (1.29 mm)

Chariklo	TPM^a, large rough.	240	0.037	N/A	8.0	This work	1.21 (1.29 mm)

Chariklo	NEATM, Maclaurin	143 × 143 × 96	0.038	1.09	N/A	This work	1.00 (1.29 mm)

						A01^b	0.81 (1.20 mm)

Chariklo	NEATM, Jacobi	160 × 142 × 88	0.041	1.04	N/A	This work	0.92 (1.29 mm)

						A01^b	0.76 (1.20 mm)

Chariklo	NEATM, Triaxial	146 × 131 × 101	0.038	1.11	N/A	This work	1.06 (1.29 mm)

						A01^b	0.87 (1.20 mm)

Chariklo, ring-corr.	NEATM	230	0.040	1.15	N/A	This work	1.21 (1.29 mm)

						A01^b	1.01 (1.20 mm)

Chariklo, ring-corr.	NEATM, Jacobi	154 × 136 × 84	0.041	1.00	N/A	This work	0.89 (1.29 mm)

						A01^b	0.71 (1.20 mm)

Notes.

^(a)

TPM: thermophysical model.

^(b)

A01: Altenhoff et al. (2001).

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