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Table 1.

Best-fit parameters of the geometric models in the L band.

Ring models

Object Rin θ i PA p fbg0 fstar0 dbg dring
(mas) (mas) (deg) (deg) (%) (%)
HD 101584 0.7 1.9 ± 0.1 6.5 ± 0.6 23 ± 17 18 ± 21 −3.0 ± 0.3 11 ± 9 2 34.1 ± 10.0 24.9 ± 6.8
HD 108015 ( * ) 9.0 1.7 ± 0.3 8.1 ± 1.7 35 ± 11 45 ± 13 −1.4 5 ± 1 10 −15.4 ± 3.7 4.2 ± 3.8
IRAS 08544 23 5.8 ± 0.1 7.9 ± 0.9 16 ± 5 116 ± 25 −1.6 37 ± 1 6 2.8 ± 1.4 −0.8 ± 0.8
IRAS 15469 1.0 1.7 ± 0.2 14.8 ± 2.3 47 ± 5 50 ± 4 −2.1 11 ± 3 6 −1.1 ± 5.3 −1.5 ± 5.8
IW Car ( * ) 29 2.2 ± 0.2 18.2 ± 1.1 50 ± 3 172 ± 2 −1.1 ± 0.1 11 ± 1 2 34.2 ± 5.4 34.9 ± 5.3
CT Ori ( * ) 1.5 3.9 ± 0.2 2.1 ± 1.0 40 ± 4 172 ± 5 −1.5 ± 0.3 20 ± 3 29 2.9 ± 1.8 −0.4 ± 1.8
AD Aql 0.5 2.2 ± 0.5 2.8 ± 1.3 39 48 ± 19 −2 27 ± 11 37 8.3 ± 2.1 12.5 ± 3.7
RU Cen 1.6 3.1 ± 0.4 0.9 ± 0.5 68 ± 8 154 ± 5 −2 9 ± 2 78 9.2 ± 1.6 −6.3 ± 3.1
ST Pup 15 1.5 ± 0.6 9.8 50 128 −1.6 30 ± 5 61 6.2 ± 1.0 15 ± 12

Binary models

Object fbg0 fstar fstar2 dbg xstar2 ystar2
(%) (%) (%) (mas) (mas)

EP Lyr 2.3 18 ± 17 65 ± 12 17 ± 14 2.3 ± 2.1 −0.1 ± 0.3 1.6 ± 0.8

Notes. Reported values are calculated at λ0 = 3.5 μm. ( * )The model included azimuthal modulations.

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