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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 3.

Top panel shows the phase-averaged and background-subtracted spectra above 3.5 keV of 4U 1626−67 obtained with Suzaku XIS (FI: black crosses, BI: light gray crosses) and HXD (gray circles). The lower four panels show the residuals in units of standard deviations, χ, from fitting by (a) the NPEX with GABS model without Fe-line emission model, (b) the NPEX with GABS model and Fe-line emission model, (c) the NPEX with CYAB and Fe-line emission model, and (d) the ECUT with GABS model and Fe-line emission model.

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