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XRISM/Resolve Reveals the Profiles of Neutral Iron Emission Lines in an Outburst X-Ray Spectrum of the Be/X-Ray Binary Pulsar 1A 1118-61

  • Authors: Toshihiro Takagi, Megumi Shidatsu, Motoki Nakajima, Mutsumi Sugizaki, Tatehiro Mihara, Camille M. Diez, Gabriele A. Matzeu, Simon Dupourqué

Toshihiro Takagi et al 2026 The Astrophysical Journal Letters 1009 .

  • Provider: AAS Journals

Caption: Figure 4.

(Top) Pulse-phase-averaged Resolve spectrum in the 6.2–7.2 keV range. The blue and red solid lines indicate the best-fit model using Model 1 and Model 2, respectively. The contributions of the narrow and broad Fe Kα components for Model 2 are also shown as green dashed lines. The middle and bottom panels show residuals between the data and the models in the cases of Model 1 and Model 2, respectively. The error bars represent 1σ statistical uncertainty.

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