Volume 532, August 2011
|Number of page(s)||5|
|Published online||21 July 2011|
Flux, squared visibility amplitude, closure phase, and uniform disk diameter (from top to bottom) as a function of wavelength for the Mira variables X Hya, W Vel, and RW Vel (from left to right). As Fig. 1, but for the remaining targets of our sample.
|Open with DEXTER|
© ESO, 2011
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