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Paper detail

The eclipse timings of RR Lyncis

The times of minima of the bright, eccentric eclipsing binary RR Lyncis are re-investigated. From the TESS data it is found that significant differences in the eclipse timings, particularly for the primary minima, are probably due to small, irregular changes in the eclipse profile due to pulsations, rather than light-curve asymmetries.

preprint2022arXivOpen access
Christopher Lloyd
astro-ph.SR
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Christopher Lloyd

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