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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. 6.

Top panel: Long‐term I light curve of RX J0103.6−7201 (SXP1323). Second panel: Periodogram of ﹩I^{*}﹩ data showing several significant periods and their aliases (see text). Third panel: ﹩I^{*}﹩ data folded on ﹩P=0.96﹩ days after signals from ﹩P=0.88﹩ and 0.42 days have been subtracted. Fourth panel: ﹩I^{*}﹩ data folded on ﹩P=0.88﹩ days after the variation of the other two NRPs has been subtracted. Bottom panel: Similar to the above two panels, but the ﹩I^{*}﹩ data have been folded on ﹩P=0.42﹩ days after subtraction of the variation due to the two other short periods.

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