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SPECTRAL ANALYSIS IN ORBITAL/SUPERORBITAL PHASE SPACE AND HINTS OF SUPERORBITAL VARIABILITY IN THE HARD X-RAYS OF LS I +61°303

  • Authors: Jian Li, Diego F. Torres, and Shu Zhang

Li, Torres, & Zhang 2014 The Astrophysical Journal Letters 785 L19.

  • Provider: AAS Journals

Caption: Figure 3.

Left: superorbital light curve of LS I +61°303 in 18–60 keV, as observed by INTEGRAL. The red points show the modulated fraction in the 3–30 keV band from Li et al. (2012). Middle and bottom: exposure and significance for the corresponding superorbital phase, respectively. Right: radio flux intensity at 2.25 GHz (top) and spectral index (bottom) as a function of the orbital and superorbital phases.

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