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TRIMOR - three-dimensional correlation technique to analyse multi-order spectra of triple stellar systems: application to HD 188753

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Academic year: 2021

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Figure

Figure 1. Orbital solution for HD 188753. The circles refer to A, triangles to Ba and squares to Bb
Figure 2. The residuals of the orbital solution in Fig. 1. The rms for A is 98 m s − 1 , for Ba is 71 m s − 1 and for Bb is 0.5 km s − 1 .
Figure 4. For each assumed mass of the Ba component, the plot shows the derived K s magnitude (in the 2MASS K s band), assuming the known mass ratio q B , and the known distance modulus of 3.31

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