Fedele, DWittkowski, MParesce, FScholz, MichaelWood, Peter RCiroi, S2015-12-082015-12-089783540742531http://hdl.handle.net/1885/33160We present near-infrared K-band interferometric measurements of the Mira star R Leonis obtained in April 2001 and January 2002 with VLTI/VINCI. The April 2001 measurements indicate a center-to-limb intensity variation (CLV) that is clearly different from200810.1007/978-3-540-74256-2_102015-12-08