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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. 5.

Top: Long‐term V (upper) and I (lower) light curves of CXOU J010102.7−720658 (SXP304). Middle: Periodograms of ﹩V^{*}﹩ data from four time segments (A–D) showing the variation in period and power. Bottom: Folded light curve of ﹩V^{*}﹩, ﹩R^{*}﹩, and ﹩I^{*}﹩ data from segment C showing strong NRPs at ﹩P=0.26﹩ days. The amplitude appears to be greatest in ﹩V^{*}﹩.

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