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[en] The star RZ Guis is confirmed as a cataclysmic variable. Its ultraviolet spectrum suggests that it belongs to the UX UMa subclass in which an optically thick disc is maintained at outburst state; coordinated optical and UV photometry show changes of about one magnitude on a time-scale of months in addition to smaller variations on a scale of minutes, but not the major outbursts of the dwarf novae. (author)
Journal
Monthly Notices of the Royal Astronomical Society; ISSN 0035-8711; 
; v. 206(4); p. 819-831
; v. 206(4); p. 819-831