Volume 45 number 2 (2017)
(Abstract only) Among the ~1000 known cataclysmic variables, only one appears to belong to the “Galactic halo”—the Population II stars. We report round-the-world photometry of this star (OV Boo) during March–April 2017, when it staged its first certified dwarf-nova outburst. The star is remarkable for its short binary period (66 minutes), high proper motion, metal-poor composition, substellar secondary, sharp white-dwarf eclipses, and nonradial pulsations. Something for everybody—and it even had the good manners to erupt in northern springtime, when it transits near local midnight. Move over, SS Cyg and WZ Sge; there’s a new celebrity in town!