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Photometric Variability of Be/X‐Ray Pulsar Binaries in the Small Magellanic Cloud

  • Authors: P. C. Schmidtke and A. P. Cowley

Schmidtke & Cowley 2006 The Astronomical Journal 132 919.

  • Provider: AAS Journals

Caption: Fig. 1.

Top: Long‐term I light curve of XMMU J005152.2−731033 (SXP172). Middle: Variance calculated by the PDM method (upper, with scale on right) and periodogram (lower) of ﹩I^{*}﹩ data from segment A. The 99% confidence level is also shown. Bottom: ﹩I^{*}﹩ data folded on the 69.9 day period and binned (squares), with the individual points from the outburst near MJD 50,790 superposed (circles).

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