Period analysis of two non-Blazhko RRab stars, FN Lyr and V894 Cyg, based on Kepler photometry: evidence of low-mass companions on wider orbits
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/444/1/600/18501670/stu1344.pdf
Reference37 articles.
1. Flavours of variability: 29 RR Lyrae stars observed with Kepler
2. First CoRoT light curves of RR Lyrae stars
3. Period and light-curve fluctuations of the Kepler Cepheid V1154 Cygni
4. Origins of Eccentric Extrasolar Planets: Testing the Planet‐Planet Scattering Model
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1. RR Lyrae from binary evolution: abundant, young, and metal-rich;Monthly Notices of the Royal Astronomical Society;2023-12-23
2. Two Different Weak Modulations in ab-type RR Lyrae Variable V838 Cyg, and Potential Influence of Metal Abundance on Blazhko Modulation;The Astronomical Journal;2023-08-01
3. Time series analysis of brightTESSRRc stars: additional modes, phase variations, and more;Monthly Notices of the Royal Astronomical Society;2023-02-21
4. Reanalysis of c-type RR Lyrae variable BE Dor, period modulations and possible mechanism;Monthly Notices of the Royal Astronomical Society;2022-02-01
5. Is the eclipsing binary RR Dra dancing with a hidden tertiary black hole candidate?;Monthly Notices of the Royal Astronomical Society;2021-08-19
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