Fig. 2 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. 2.

Background‐subtracted PCA and HEXTE spectra of 4U 0115+63 in the 1999 outburst, shown normalized to those of the Crab Nebula measured by the respective instruments. The figure excludes second observations on the same date (March 19b, 21b) and low‐exposure data (March 16 and 18 and April 1).

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