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RXTE Discovery of Multiple Cyclotron Lines during the 2004 December Outburst of V0332+53

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Published 2005 November 2 © 2005. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Katja Pottschmidt et al 2005 ApJ 634 L97 DOI 10.1086/498689

1538-4357/634/1/L97

Abstract

We present an analysis of the 2-150 keV spectrum of the transient X-ray pulsar V0332+53 taken with the Rossi X-Ray Timing Explorer (RXTE) in 2004 December. We report on the detection of three cyclotron resonance features at 27, 51, and 74 keV in the phase-averaged data, corresponding to a polar magnetic field of 2.7 × 1012 G. After 4U 0115+63, this makes V0332+53 the second accreting neutron star in which more than two cyclotron lines have been detected; this has now also been confirmed by INTEGRAL. Pulse-phase spectroscopy reveals remarkably little variability of the cyclotron line through the 4.4 s X-ray pulse.

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10.1086/498689