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BE Lyncis: A Pulsating Star in the Most Eccentric Binary with a Massive Unseen Companion

  • Authors: Jia-Shu Niu, 家树 牛, Ying Zhang, 颖 张, Hui-Fang Xue, 会芳 薛

Jia-Shu Niu et al 2026 The Astrophysical Journal Letters 1001 .

  • Provider: AAS Journals

Caption: Figure 1.

O − C diagram of BE Lyn (with the linear ephemeris subtracted). The top panel shows the data and the best-fit model (magenta solid line), with the quadratic component indicated by the green dashed line. The bottom panel displays the residuals. Data sources are color-coded: C. Boonyarak et al. (2011; blue), historical literature (J. Hubscher et al. 2013; J. Hubscher 2014; J. H. Peña et al. 2015; J. Hübscher 2017; L. Pagel 2021, 2022, 2023; gray), AAVSO (red), and TESS (green).

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