Fig. 5 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. 5.

PCU ﹩0+2+3﹩ light curve of 4U 0115+63 observed from March 27 to April 8, plotted with 16 s binnings. The horizontal dashed lines indicate boundaries of the intensity sorting.

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