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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. 4.

(a) Date‐sorted PCA spectra of 4U 0115+63 from March 27 to April 8, normalized to the respective best‐fit NPEX models. For the presentation, the results are shifted vertically by a factor of 0.5 for each observation. (b) Same as (a), but the fitting model is NPEX×CYAB2 (March 27 through April 2) or NPEX×CYAB (April 4 and later).

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