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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 Journal 646 1125.

  • Provider: AAS Journals

Caption: Fig. 3.

Pulse‐phase–averaged spectra of 4U 0115+63 on March 27 (left) and April 8 (right). (a, e) Background‐subtracted spectra of the PCA and HEXTE, shown in comparison with the best‐fit NPEX×CYAB model (histograms). Two resonances are incorporated to fit the March 27 data, but only a single resonance for the April 8 data. (d, g) Ratios from the NPEX model fits. (b, c, g) Ratios from the NPEX model with (b) triple, (c) double, and (f) single CRSF.

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