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Contemporaneous Ultraviolet and Optical Observations of Direct and Raman‐scattered O<scp>vi</scp>Lines in Symbiotic Stars
Symbiotic stars are binary systems consisting of a hot star, typically a white dwarf, and a cool giant companion. The wind from the cool star is ionized by the radiation from the hot star, resulting in the characteristic combination of sharp nebular emission lines and stellar molecular absorption bands in …