Volume 583, November 2015
|Number of page(s)||14|
|Published online||02 November 2015|
Journal of the MIDI observations of RU Vir.
Comparison of the observational MIDI data with the best-fitting geometrical model (see Table 3). Shown are visibilities vs. wavelength at different position angles and baseline lengths (see Fig. 3 for the complete set of visibilities). Black lines represent the MIDI observations of RU Vir. Light blue lines represent the fit of the best-fitting UD+Gaussian model.
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© ESO, 2015
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