USNO-B1.0 1171-0309158: An RR Lyrae Star that Switched from a Double- to   Single-mode Pulsation
  We report the discovery of a new case of an RR Lyrae star that experienced a switching of its pulsation mode. We detected USNO-B1.0 1171-0309158 as a double-mode RR Lyrae star from observations of the Catalina surveys (CSS) that showed additional scattering on the light curve. Our analysis of the time-series of CSS data showed gradual increase in scattering and in the amplitude of fundamental pulsation mode. Our CCD observations carried out in 2015 reveal that this object is now a fundamental-mode RRab star, with no sign of the first-overtone pulsation. 
A.V. Khruslov, A.V. Kusakin, I.V. Reva
astro-ph.SR