RXTE confirmation of the intermediate polar status of Swift J0732.5-1331

16Citations
Citations of this article
5Readers
Mendeley users who have this article in their library.

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.

Cite

CITATION STYLE

APA

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

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free