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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 3.

Top: inferred blackbody radius R bb (filled points) plotted over fitted double-exponential model luminosity (gray), folded within each epoch. The short-term evolution is consistent with a cooling emission region expanding by a factor of ∼2–3 over each flare, in agreement with Miniutti et al. (2023b). Over the long term, the peak inferred R bb appears to grow (from 2020 August to 2022 February), then shrinks (by 2022 October–November). This may be a geometric (viewing-angle) effect attributed to the EMRI apsidal precession (∼10s of days), or a change in the mutual EMRI-disk inclination due to the EMRI nodal precession (∼100s of days) resulting in changing ejecta properties (see discussion in Section 4.2). Bottom: same plot for kT.

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