http://arxiv.org/abs/1703.03029
Over the recent years, the Petersen diagram for classical pulsators, Cepheids and RR Lyr stars, populated with a few hundreds of new multiperiodic variables. We review our analyses of the OGLE data, which resulted in the significant extension of the known, and in the discovery of a few new and distinct forms of multiperiodic pulsation. The showcase includes not only radial mode pulsators, but also radial-non-radial pulsators and stars with significant modulation observed on top of the beat pulsation. First theoretical models explaining the new forms of stellar variability are briefly discussed.
R. Smolec, W. Dziembowski, P. Moskalik, et. al.
Fri, 10 Mar 17
8/52
Comments: 5 pages; to be published in the proceedings of the 22nd Los Alamos Stellar Pulsation Conference “Wide-field variability surveys: a 21st-century perspective”, San Pedro de Atacama, Chile, Nov. 28 – Dec. 2, 2016