Fig. 4 from ASCA Observation of the Dipping X‐Ray Source XB 1916−053

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ASCA Observation of the Dipping X‐Ray Source XB 1916−053

Authors: Yuan-Kuen Ko, Koji Mukai, Alan P. Smale, and Nick E. White

Ko et al. 1999 The Astrophysical Journal 520 292.

Provider: AAS Journals

Caption: Fig. 4.

GIS‐combined folded light curves in two different energy ranges: 0.6–1.5 keV (top) and 3–10 keV (middle). Bottom: The hardness ratio (3–10 keV/0.6–1.5 keV) of the GIS‐combined folded light curves. The ratio increases during the primary and secondary dips.

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