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A Double Outburst from IGR J00291+5934: Implications for Accretion Disk Instability Theory

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Academic year: 2021

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Figure

Figure 1. RXTE PCA light curve of the 2008 outbursts from IGR J00291+5934.
Figure 2. Light curves, phases, and fractional amplitudes of the observed outbursts of IGR J00291+5934
Figure 3. Light curve for the first 7 days of the 2004 outburst and a comparison the best-fit linear (solid line) and exponential (dashed line) models
Figure 4. Spectral fits for the three outbursts. The 2.5–25 keV flux from IGR J00291+5934 is shown for reference, in units of 10 −10 erg cm −2 s −1
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