AbstractWe report on the luminosity dependent change of the cyclotron resonance energy obtained from a transient X-ray pulsar, 4U 0115+63. Using RXTE data observed on 1999 March, we found that the fundamental resonance energy stayed constant (∼11keV) when the source luminosity was above ∼5×1037ergs−1. As the luminosity decreased below ∼5×1037ergs−1, the fundamental resonance energy gradually increased up to ∼16keV at 0.16×1037ergs−1. The luminosity dependence of the resonance energy can be understood by the change of the accretion column height.


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    Title :

    Study of the luminosity-dependent cyclotron resonance energies of the binary X-ray pulsar 4U 0115+63 with RXTE


    Contributors:
    Nakajima, M. (author) / Mihara, T. (author) / Makishima, K. (author) / Niko, H. (author)

    Published in:

    Advances in Space Research ; 38 , 12 ; 2756-2758


    Publication date :

    2005-09-01


    Size :

    3 pages




    Type of media :

    Article (Journal)


    Type of material :

    Electronic Resource


    Language :

    English