Á. Juhász, L. Molnár, E. Plachy
Published 2016-03-29Version 1
We have started a comprehensive analysis of the Kepler K2 Field 3 data set. Our goals are to assess the statistics of the sample, and to search for peculiar stars. We found a candidate triple-mode RRab star, where the first and ninth overtones also seem to be excited.
Comments: Comments: 2 pages, 1 figure, proceedings of the RRL2015 - High-Precision Studies of RR Lyrae Stars conference, to appear in the Communications from the Konkoly Observatory
On a new theoretical framework for RR Lyrae stars I: the metallicity dependence
Metallicity estimation of RR Lyrae stars from their I-band light curves
Over 78 000 RR Lyrae Stars in the Galactic Bulge and Disk from the OGLE Survey
![QR code for arXiv:1603.08671 [astro-ph.SR]](http://oss.arxitics.com/images/favicon.svg)