Millimetre continuum from luminous blue variable stars and their environs - NIKA2 observations and Virtual Observatory data

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Table 3

Best-fit model results.

Source	T_eff	R_star	$A_{g}^{i s m}$ $\[A_{\mathrm{g}}^{\mathrm{ism}}\]$	$A_{g}^{c s m}$ $\[A_{\mathrm{g}}^{\mathrm{csm}}\]$	T_dust	R_dust	M_dust	$\dot{M}$ $\[\dot{M}\]$ ^(a)	n_e	R_ff
	10³ K	R_⊙	mag	mag	K	au	M_⊙	10⁻⁶ M_⊙ yr⁻¹	cm⁻³	10³ au
HD 168607	17 ± 1	100 ± 10	4.71	1.6	1100 ± 100	3 ± 1	6.4 × 10⁻⁶	1.0 ± 0.3
					35 ± 5	85 ± 5	5.1 × 10⁻³
HD 168625	11 ± 1	80 ± 10	1.13	4.2	500 ± 100	21 ± 1	3.1 × 10⁻⁴		2 ± 1 × 10⁴	1.2 ± 0.2
					140 ± 20	^_(b)	2.0 × 10⁻³		2 ± 1 × 10⁴	1.2 ± 0.2
MN101	11 ± 1	70 ± 10	7.56	8.3	1800 ± 200	1.5 ± 0.5	1.6 × 10⁻⁶		8 ± 2 × 10³	3.2 ± 0.4
					100 ± 20	160 ± 20	7.1 × 10⁻³		8 ± 2 × 10³	3.2 ± 0.4
G79.29+0.46	18 ± 1	80 ± 10	9.96	5.2	1100 ± 100	2 ± 1	2.8 × 10⁻⁶	2.2 ± 0.3
					40 ± 10	90 ± 10	5.7 × 10⁻³

Notes. ^(a) A wind velocity of 100 km s⁻¹ is assumed (Appendix B). ^(b) Cannot be estimated due to opacity (see Sect. 5.1 and Appendix B).

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