Table 2: Summary of the results obtained in the case where the angular separation of the two stars is $\frac{1}{2}\lambda/D$. The quantities $\Delta m_0$, $\Delta \Theta _{\rm r} $, and $\Delta m_{\rm r}$ are defined in the text.
main star case A case B case C
K-band mag. $\Delta m_0$ $\Delta \Theta _{\rm r} $ $\Delta m_{\rm r}$ $\Delta m_0$ $\Delta \Theta _{\rm r} $ $\Delta m_{\rm r}$ $\Delta m_0$ $\Delta \Theta _{\rm r} $ $\Delta m_{\rm r}$
10 3.5 20% 3.75 3 20% 2.8 2.5 20% 2.4
12 3 10% 3.2 2.5 20% 2.5 2.5 15% 3.3
14 2.5 20% 2.5 2.5 20% 2.2 2.5 15% 3.1
15 2.5 20% 2 2 10% 1.5 2 20% 2.7
17 2 20% 1 1 20% 0.4 1 10% 0.4


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