Abstract
We discuss the prospects for resolving the disks of red-giants and Mira variables with the VLT and the VLTI. We also describe infrared aperture-masking observations with the NTT, from which we have measured angular diameters of 50 mas for R Dor (M8 III) and 44mas for W Hya (Mira variable).
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Bedding, T.R., von der Lühe, O., Zijlstra, A.A. (1995). Imaging the Surfaces of Late-Type Stars. In: Walsh, J.R., Danziger, I.J. (eds) Science with the VLT. ESO Astrophysics Symposia. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-49215-3_12
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DOI: https://doi.org/10.1007/978-3-540-49215-3_12
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