Fig. 1 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. 1.

Top: The 2–10 keV RXTE ASM light curve of 4U 0115+63 in the 1999 March–April outburst. Middle and bottom: The 3–30 keV PCA and the 15–50 keV HEXTE light curves obtained from the 33 pointing observations listed in Table 1.

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