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arxiv: 1108.4987 · v1 · pith:JHPNZUE7new · submitted 2011-08-25 · 🌌 astro-ph.SR

Peculiarities of Blazhko Stars: New Insights

classification 🌌 astro-ph.SR
keywords blazhkostarsgiverecentwhataccurateamplitudecause
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With increasingly accurate data on RR Lyrae stars we find that the Blazhko effect may be a rule rather than an exception. However, we still do not know what is the cause of this mysterious amplitude and phase modulation. In my talk, I intended to give a glimpse of the properties of Blazhko stars, presenting recent findings concerning what makes Blazhko stars different from their non-modulated counterparts. Recent observations of Blazhko stars obtained from space give some important clues that deserve further exploration.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. IY Lyr: A Thick-Disk first-overtone RR Lyrae Star with a Possible Neutron Star Companion

    astro-ph.SR 2026-05 conditional novelty 6.0

    IY Lyr is a thick-disk RRc star with a 1.37 solar-mass companion most likely a neutron star in a 3.94-year eccentric orbit, confirmed by photometry, spectroscopy, and astrometry.