Fig. 9 from 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

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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. 9.

Same as Fig. 8, but the resonance energy is converted through eq. (4) into the height (﹩h_{r}﹩) at which the resonance occurs. The dashed line represents the value of the column top height, ﹩h_{\mathrm{top}\,}﹩, calculated by eq. (5).

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