Аннотация:We present our discovery of a new double-mode high-amplitude δ Scuti variable, HADS(B) type, USNO-B1.0 1329-0132547.
We found the frequencies f0 = 6.1770 and f1 = 8.0561. The period ratio P1/P0 = 0.7668 is typical of radially pulsating HADS(B) stars.