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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 9.

Fit parameters as a function of pulse phase for 4U 1626−67. Best-fit values by NPEX with GABS model (Table 3) are plotted.

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