We report on the results of a 50 ks BeppoSAX observation of 1RXS J170849-400910, one of the five (plus a candidate) known anomalous X-ray pulsars (AXPs). The BeppoSAX data are consistent with a power-law + blackbody spectral decomposition, making 1RXS J170849-400910 the fourth source of this class for which such a spectral decomposition was found. The inferred power-law slope and blackbody temperature are Γ ∼ 2.6 and kTBB ∼ 0.46 keV, respectively. We find that the pulse profile is significantly energy-dependent, a remarkable feature for an AXP. By using the power-law + blackbody decomposition, we detect a significant variation in at least one spectral parameter, the power-law photon index, as a function of the pulse phase. This is the first significant detection of a spectral parameter variation in an AXP. The implications of these results are briefly discussed.
CITATION STYLE
Israel, G., Oosterbroek, T., Stella, L., Campana, S., Mereghetti, S., & Parmar, A. N. (2001). The Pulse-Phase–dependent Spectrum of the Anomalous X-Ray Pulsar 1RXS J170849−400910. The Astrophysical Journal, 560(1), L65–L69. https://doi.org/10.1086/324169
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