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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. 3.

Top: Long‐term R light curve of XMMU J005605.2−722200 (SXP140). Middle: Periodogram of ﹩R^{*}﹩ data from segment A showing the orbital period of 197 days. Bottom: ﹩R^{*}﹩ light curve folded on 197 days and averaged in 20 phase bins.

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