Fig. 11 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

Nakajima et al. 2006 The Astrophysical Journal 646 1125.

Caption: Fig. 11.

CRSF depth τ against the fractional width ﹩W/ E_{a}﹩. The plotted points are obtained from the date‐sorted and intensity‐sorted analyses.