Multiwavelength interferometric observations and modeling of circumstellar disks

Free Access

Table 7

Parameters of the models whose SED, NIR, and MIR visibilities are shown in Figs. 1–3.

Object	Model	M _disk	R _in	β	h ₁₀₀	i	Ṁ	f _ρ	R _gapin	R _gapout
	no.	(M_⊙)	(AU)		(AU)	(°)	(M_⊙/a)		(AU)	(AU)

HD 142666	i	0.4	0.10	1.0	11	0−50		1	–	–	1
	ii	0.4	0.50	1.0	11	0−50		1	–	–	5
	iii	0.4	0.10	1.1	11	0−50		1	–	–	3
	iv	0.4	0.50	1.0	11	0−50	7 × 10^-8	1	–	–	1
	v	0.4	0.10	1.0	11	0−50		0.01	–	–	2
	vi	0.4	0.30	1.0	11	0−50		0.01	0.35	0.80	2
	vii	0.4	0.30	1.0	11	0−50		1	0.35	0.80	3
AS 205 N		0.08	0.10	1.0−1.1	19−21	40 < i < 45		–	–	–	−8
AS 205 S		0.05	0.10	1.0	21	<45	~	–	–	–	5

Notes.The parameters of model vi of HD 142666 and the parameters of AS 205 N and AS 205 S simulate the observations best. The last column lists the ratio between the stellar and disk model flux in H band at 1.6 μm.

Reference. 1) Garcia-Lopez et al. (2006); 2) Eisner et al. (2005).

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.