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Testing EMRI Models for Quasi-periodic Eruptions with 3.5 yr of Monitoring eRO-QPE1

  • Authors: Joheen Chakraborty, Riccardo Arcodia, Erin Kara, Giovanni Miniutti, Margherita Giustini, Alexandra J. Tetarenko, Lauren Rhodes, Alessia Franchini, Matteo Bonetti, Kevin B. Burdge, Adelle J. Goodwin, Thomas J. Maccarone, Andrea Merloni, Gabriele Ponti, Ronald A. Remillard, Richard D. Saxton

Joheen Chakraborty et al 2024 The Astrophysical Journal 965 .

  • Provider: AAS Journals

Caption: Figure 7.

Overplotted even/odd burst sequences (demonstrating the high scatter and lack of any long/short recurrence pattern), and the corresponding O–C timing residuals (i.e., whether each burst arrives early/late compared to the average t rec within the epoch, Section 3.3.1). As noted in Arcodia et al. (2022), the scatter in recurrence time (∼50%) is significantly higher than other QPE sources. The O–C plots are overplotted with best-fit periods per epoch (gray dashed line) and overall (blue dashed). The 2020 August epoch (P peak = 8.96 days) and the first 2022 December epoch (P peak = 2.5 days) are significant outliers from the 5.73 average period. The long-short recurrence pattern seen in other QPEs is not generally seen in eRO-QPE1, with the possible exception of a short-lived phase in early 2022 December.

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