Abstract
RY Scuti, the 11-day [Fe III] eclipsing binary, has been reinvestigated on the basis of spectroscopic material secured at the European Southern Observatory (ESO), La Silla, Chile, and at the Cerro Tololo Interamerican Observatory (CTIO), Chile, that cover the regions 3400–5150 Å and 5700–6700 Å, and worked out with the measuring and computing facilities at the ESO Headquarters, Garching bei München, Germany. Ultraviolet observations taken with the IUE satellite were also analyzed.
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