A Further Study of the Luminosity‐dependent Cyclotron Resonance Energies of the Binary X‐Ray Pulsar 4U 0115+63 with the Rossi X‐Ray Timing Explorer
Authors: M. Nakajima, T. Mihara, K. Makishima, and H. Niko
Nakajima et al.
2006 The Astrophysical Journal6461125.
Provider: AAS Journals
Caption: Fig. 6.
(a) Same as Fig. 4a, but for the intensity‐sorted spectra defined in Fig. 5. (b) Intensity‐sorted PCA spectra, each normalized to the best‐fit NPEX×CYAB2 (f1–f5) or NPEX×CYAB (f6–f8) model. Data are presented in the same manner as in Fig. 4.
