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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. 12.

Dependence of the CRSF and NPEX parameters on the 3–50 keV luminosity, obtained from the 34 date‐sorted data sets and the 8 intensity‐sorted data sets. The circles and triangles represent those spectra that are described by the double and single CRSF factor(s), respectively. (a) The ﹩W/ E_{a}﹩ ratio for the fundamental and second harmonic resonances. (b) NPEX kT. (c) Fundamental resonance depth, ﹩\tau _{1}﹩. (d) Second harmonic depth, ﹩\tau _{2}﹩.

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