Astronomy and Astrophysics – Astrophysics
Scientific paper
2000-04-20
Astronomy and Astrophysics
Astrophysics
5 pages. To appear in "Proceedings of the 5th Compton Symposium"
Scientific paper
10.1063/1.1303197
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.
Coburn Wayne
Gruber Duane E.
Heindl William A.
Pelling Michael
Pottschmidt Katja
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