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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 6.

Pulse profile (top; same as Figure 2) and variations in the Fe Kα and Kβ line spectral parameters as a function of pulse phase, obtained from the best-fit models in Table 2: (A) redshift z, (B) broadening width σ, (C) normalization (flux), and (D) EW. The black circles, red squares, and blue triangles represent the parameters for the narrow Fe Kα, broad Fe Kα, and narrow Fe Kβ lines, respectively. For clarity, the marker positions of the circles and triangles are slightly shifted along the X-axis. Note that the z-values for the Fe Kβ line are the sum of the two zashift model parameters (i.e., the total redshift from the rest frame).

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