Circumstellar disks around Herbig Be stars | Astronomy & Astrophysics (A&A)

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This article has an erratum: [https://doi.org/10.1051/0004-6361/200810401e]

Table 6:

Envelope modeling results.
Name	Dust mass	Inner radius	Outer radius	Density	Inner temperature	Geometry	Inclination
	( $M_\odot$ )	(AU)	(AU)	slope	(K)		(degrees)
MWC 137	0.005	5000.0	11 700.0	-1.0	61	Sphere
R Mon	0.008	700.0	12 000.0	-1.4	62	Toroid¹	70.0
MWC 1080	0.025	6000.0	12 000.0	-1.0	44	Toroid	80.0
Z CMa	0.05	2000.0	5000.0	-0.6	42	Toroid¹	30.0
LKH $\alpha$ 215	0.0015	3500.0	7200.0	0.0	57	Sphere

¹ The dust temperature in the envelope is assumed to be described by a power law, $T(r) = T_{\rm in} (r/r_{\rm in})^{-0.5}$ .
See Sects. 4 and 5 for a more detailed discussion.

Source LaTeX | All tables | In the text

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