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Possible Detection of an Emission Cyclotron Resonance Scattering Feature from the Accretion-powered Pulsar 4U 1626–67

  • Authors: W. B. Iwakiri, Y. Terada, T. Mihara, L. Angelini, M. S. Tashiro, T. Enoto, S. Yamada, K. Makishima, M. Nakajima, and A. Yoshida

Iwakiri et al. 2012 The Astrophysical Journal 751 35.

  • Provider: AAS Journals

Caption: Figure 8.

Upper panel shows spectra in the dim phase (ϕ = 0.125–0.250) of 4U 1626−67 obtained with Suzaku XIS (FI: black crosses, BI: light gray crosses) and HXD (circles). Triangles denote the reproducibility of NXB for HXD-PIN. Histograms in the upper panel are the best-fit by NPEX continuum ( A p = 0). The lower three panels show residuals, χ, when fitting by (a) NPEX ( A p = 0) continuum-only, (b) NPEX ( A p = 0) with GABS model, and (c) NPEX ( A p = 0) and Gaussian models.

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