Luminosities and mass-loss rates of SMC and LMC AGB stars and red supergiants

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Table 3:

Fit results of the C-star sample for the first few entries.
Identifier	$T_{\rm eff}$	grain	L	$\dot{M}$	fit?	$T_{\rm c}$	fit?	$R_{\rm out}$	$\tau_{0.5}$	$\tau_{11.3}$
	(K)	type	( $L_{\odot}$ )	( $M_{\odot }$ yr^-1)		(K)
iras04496	2800	sic0	35690	5.18e-06	1	1000	0	10000.0	4.646	0.145
iras05278	3600	sic0	30617	2.85e-05	1	1055	0	6000.0	22.645	0.704
iras00554	3600	sic4	27127	1.42e-05	1	1204	0	10000.0	16.465	0.752
msxlmc1298	3600	sic4	24506	1.15e-05	1	1142	0	41.2	12.977	0.593
msxlmc775	3200	bsic2	20776	5.59e-06	1	1082	1	4.6	7.170	0.284

sic refers to $\alpha$ -SiC from Pégourié (1988), bsic to $\beta$ -SiC from Borghesi et al. (1985). The number refers to the percentage of SiC. The rest is amorphous carbon from Rouleau & Martin (1991; also see Sect. 3).

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