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Multiple Cyclotron Lines in the Spectrum of 4U 0115+63

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arxiv astro-ph/0004297 v1 pith:KTL2ADW7 submitted 2000-04-20 astro-ph

W. A. Heindl , W. Coburn , D. E. Gruber , M. Pelling , R. E. Rothschild , J. Wilms , K. Pottschmidt , R. Staubert This is my paper · ORCID
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keywords linephasepulsarspectrumaccretingagreementappearscomplex
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We report phase resolved spectroscopy of the transient accreting pulsar, 4U0115+63. For the first time, more than two cylotron resonance scattering features are detected in the spectrum of an X-ray pulsar. The shape of the fundamental line appears to be complex, and this is in agreement with predictions of Monte-Carlo models. As in other pulsars, the line energies and optical depths are strong functions of pulse phase. One possible model for this is an offset of the dipole of the neutron star magnetic field.

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  1. Real-time observations of the transition to the quiescent state in an accreting magnetised neutron star: No propeller required?

    astro-ph.HE 2026-08 conditional novelty 6.0 of 10

    First high-cadence observation of an X-ray pulsar transition to quiescence shows a gradual exponential fade consistent with the disc instability model, without requiring the propeller effect.

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