Characterising the orbit and circumstellar environment of the high-mass binary MWC 166 A

Open Access

Fig. 8.

Radial velocity measurements of MWC 166 A taken in the period 1994–2005 plotted against orbital phase. The blue and red fitted curves correspond to the orbits specified in Cols. (3) and (4) of Table 4, respectively. The dotted black line shows the velocity of the system’s centre of mass (V₀) for the grid-search method, and the solid grey line shows V₀ for the ORBITX orbit.

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