Detailed high-energy characteristics of AXP 1RXS J170849-400910 - Probing the magnetosphere using INTEGRAL, RXTE and XMM-Newton
P.R. den Hartog (1), L. Kuiper (1), W. Hermsen (1,2) ((1) SRON, Netherlands Institute for Space Research; (2) Astronomical Institute)

TL;DR
This study provides a comprehensive analysis of the spectral and temporal X-ray characteristics of AXP 1RXS J170849-400910 using data from INTEGRAL, RXTE, and XMM-Newton, revealing complex pulse components and phase-dependent spectral changes.
Contribution
It offers the first detailed phase-resolved spectroscopy of this AXP, identifying three distinct spectral components with unique pulse profiles and stability over time.
Findings
The hard X-ray spectrum extends up to ~175 keV with no spectral break.
Pulsed emission is detected up to 270 keV with high significance.
Three distinct pulse components with different spectral shapes and phase distributions are identified.
Abstract
We present detailed spectral and temporal characteristics over the whole X-ray band. For this purpose data have been used from INTEGRAL, RXTE and XMM-Newton. The INTEGRAL hard X-ray (>10 keV) time-averaged total spectrum, can be described by a power law with a photon index Gamma = 1.13 +/- 0.06 and extends to ~175 keV. No evidence for a spectral break is found. No significant long-term time variability has been detected above 20 keV. Pulsed emission is measured up to 270 keV (12.3 sigma; 20-270 keV). Three different pulse components can be recognized in the pulse profiles: 1) a hard pulse which contributes above ~4 keV, 2) a softer pulse not contributing in the hard X-ray domain and 3) a very soft pulse component below 2 keV. Detailed phase-resolved spectroscopy of the pulsed emission confirms long-term stability. The spectral shape gradually changes with phase from a soft single power…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Pulsars and Gravitational Waves Research · High-pressure geophysics and materials
