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No Evidence for a Supermassive Black Hole Binary in GSN 069

  • Authors: Yuhe Zeng, Zhen Pan, Bin Liu, Cong Zhou

Yuhe Zeng et al 2026 The Astrophysical Journal Letters 1011 .

  • Provider: AAS Journals

Caption: Figure 1.

Time intervals between adjacent eruptions of GSN 069 (G. Miniutti et al. 2019). There are clearly two antiphase branches, denoted as Teven(t) and Todd(t), where both of them vary with a period ≈76 d, while the sum Teven(t) + Todd(t) ≈ 65 ks (C. Zhou et al. 2025a, 2025b). No evidence for an in-phase modulation in even and odd eruptions is revealed.

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