VLTI/MIDI observations of 7 classical Be stars | Astronomy & Astrophysics (A&A)

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Table 4:

Stellar parameters adopted in this work and resulting 8 and 12 $\mu$ m envelope flux.
	Adopted stellar parameters					$F_{\rm e}$ ( $\%$ )
Name	$T_{\rm eff}$ (K)	log g	$R_{\rm\star}$ ( $R_{\rm\odot}$ )	d (pc)	$A_{\rm v}$	8 $\mu$ m	12 $\mu$ m
$\kappa$ CMa	24 600	4.07	5.9	202	0.37	$90\pm6$	$94\pm4$
$\delta$ Cen	22 360	3.92	6.5	127	0.10	$88\pm5$	$93\pm3$
$\alpha$ Ara	18 044	3.99	4.5	81	0.10	$87\pm4$	$91\pm3$
p Car	17 389	3.52	6.0	148	0.05	$87\pm4$	$91\pm3$
$\zeta$ Tau	19 340	3.52	7.5	136	0.30	$80\pm6$	$86\pm5$
$\alpha$ Col	12 963	3.73	5.8	80	0.00	$67\pm11$	$76\pm8$
$\beta$ CMi	11 772	3.51	3.5	49	0.00	$59\pm13$	$69\pm10$

Source LaTeX | All tables | In the text

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