Chromospherically active binary stars.

Physics

Scientific paper

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Scientific paper

Background information is provided on both low and high dispersion IUE spectra of chromospherically active late-type binaries, that have been taken until the end of 1992, in order to foster an optimum usage of the IUE archive. Physical information on all systems, arranged by binary star name, together with characteristics of the individual exposures, the position of the observations in the orbital light curve, an average low resolution ultraviolet spectrum, and, whenever available, the shape of the Mg II feature at 2800 Å in high resolution, are given.

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