Fig. 10 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. 10.

Spectral changes associated with a 1 mHz QPO observed on March 31. Top: Background‐subtracted PCA spectra accumulated at peaks and bottoms of the QPO, as specified on the 2–30 keV light curve (inset). Middle: Residuals from NPEX fits to the two spectra. Bottom: QPO bottom‐to‐peak ratio.

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