Berdnikov, L. N.L. N.BerdnikovKniazev, A. Y.A. Y.KniazevKravtsov, V. V.V. V.KravtsovDambis, A. K.A. K.Dambis2026-10-192026-10-192017-06Berdnikov, L. N.; Kniazev, A. Y.; Kravtsov, V. V.; Dambis, A. K. (2017-06). ASAS 160125-5150.3-the second galactic classical Cepheid with strong Blazhko effect. ASTROPHYSICS AND SPACE SCIENCE, 362 (6), 105. https://doi.org/10.1007/s10509-017-3088-x0004-640X1572-946Xhttps://hdl.handle.net/20.500.12740/25188In 2005-2014 we acquired a total of 135, 137 and 134 measurements in B-, V -and I-c-filters, respectively, for the 5-days Cepheid ASAS 160125-5150.3. Our observations showed variations of light amplitude, which allowed us to suspect the presence of the Blazhko effect. Combining our measurements with ASAS-3 data allowed us to determine the period of the Blazhko effect P-Bl = 1242(d) +/- 10(d), and now ASAS 160125-5150.3 is the second Galactic Cepheid (after V473 Lyr) with strong Blazhko effect pulsating in the first overtone.enVariable starsPhotometryCepheidsBlazhko effectArticulohttps://doi.org/10.1007/s10509-017-3088-x