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A Positive Period Derivative in the Quasiperiodic Eruptions of ZTF19acnskyy

  • Authors: Joheen Chakraborty, Saul A. Rappaport, Riccardo Arcodia, Itai Linial, Giovanni Miniutti, Kevin B. Burdge, Jorge Cuadra, Margherita Giustini, Lorena Hernández-García, Erin Kara, Claudio Ricci, Paula Sánchez-Sáez, Philippe Yao

Joheen Chakraborty et al 2026 The Astrophysical Journal Letters 1001 .

  • Provider: AAS Journals

Caption: Figure 3.

Left: O − C diagram of the QPEs overplotted with models 1–4. The data are consistent with P0 ≈ 9.5 days and ﹩\dot{P}\approx 1.7\times 1{0}^{-2}﹩ day day−1 at T0 ≈ 60710.1. In principle, it is possible that the apparent period increase is due to a long-term period oscillation observed locally (models 2 and 4); the > 1 yr data baseline over which ﹩\dot{P}﹩ is constant constrains any such oscillation to have a period ≳11 yr and amplitude ≳1000 days. Right: data−model residuals. Models 1–2 show structured residuals, which models 3–4 interpret as a sine with period ∼155 days and amplitude ∼0.8 days (though see Appendix).

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