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The Accreting Millisecond X-ray Pulsar IGR J00291+5934: Evidence for a Long Timescale Spin Evolution

  • Authors: Alessandro Patruno

PATRUNO 2010 The Astrophysical Journal 722 909.

  • Provider: AAS Journals

Caption: Figure 2.

X-ray flux vs. pulse phase correlation for the 2004 and the two 2008 outbursts. All three outbursts follow a correlation between flux and phase which is consistent in all three cases, within the statistical errors. The correlation has been fit with a linear relation between flux and pulse phase. The pulse phase shifts by almost 0.2 cycles during 2004 and by ~0.1 cycle during 2008, for both outburst episodes. The fit parameters and the χ 2 of the fit are reported in Table 6.

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