Abstract
Aims. We intend to establish the X-ray properties of Swift J0732.5-1331 and therefore confirm its status as an intermediate polar. Methods. We analysed 36 240 s of X-ray data from RXTE. Frequency analysis was used to constrain temporal variations and spectral analysis used to characterise the emission and absorption properties. Results. The X-ray spin period is confirmed to be 512.4(3) s with a strong first harmonic. No modulation is detected at the candidate orbital period of 5.6 h, but a coherent modulation is present at the candidate 11.3 h period. The spectrum is consistent with a 37 keV bremsstrahlung continuum with an iron line at 6.4 keV absorbed by an equivalent hydrogen column density of around 1022 atoms cm-2. Conclusions. Swift J0732-1331 is confirmed to be an intermediate polar. © ESO 2007.
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Butters, O. W., Barlow, E. J., Norton, A. J., & Mukai, K. (2007). RXTE confirmation of the intermediate polar status of Swift J0732.5-1331. Astronomy and Astrophysics, 475(2). https://doi.org/10.1051/0004-6361:20078700
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