The Blazhko Effect
arXiv:0908.4536 · doi:10.1063/1.3246458
Abstract
Current status of (the lack of) understanding Blazhko effect is reviewed. We focus mostly on the various components of the failure of the models and touch upon the observational issues only at a degree needed for the theoretical background. Attention is to be paid to models based on radial mode resonances, since they seem to be not fully explored yet, especially if we consider possible non-standard effects (e.g., heavy element enhancement). To aid further modeling efforts, we stress the need for accurate time-series spectral line analysis to reveal any possible non-radial component(s) and thereby let to include (or exclude) non-radial modes in explaining the Blazhko phenomenon.
12 pages, 3 figures, paper presented at a conference held in Santa Fe, NM, USA, May 31 - June 5, 2009. To appear in 'Stellar Pulsation: Challenges for Theory and Observation', AIP, Eds.: J. Guzik and P. Bradley
Cited by in corpus (10)
- Metal Abundances, Radial Velocities and other Physical Characteristics for the RR Lyrae Stars in the Kepler Field
- First Kepler results on RR Lyrae stars
- Long time-scale behavior of the Blazhko effect from rectified Kepler data
- Bright Blazhko RRab Lyrae stars observed by ASAS and the SuperWASP surveys
- On the modulation of RR Lyrae stars in the globular cluster M3
- The all-sky GEOS RR Lyr survey with the TAROT telescopes. Analysis of the Blazhko effect
- Frequency analysis of OGLE-IV photometry for classical Cepheids in Galactic fields: non-radial modes and modulations
- Multi-Mode Oscillations in Classical Cepheids and RR Lyrae-Type Stars
- Analysis of the possible Blazhko-effect Cepheid V473 Lyrae
- Blazhko effect in Cepheids and RR Lyrae stars