Abstract
Aims. We determine the nature of the intermediate polar candidates XSS J00564+4548, IGR J17195-4100, and XSS J12270-4859.Methods. Pointed RXTE observations searched for intermediate polar characteristics in these candidate systems.Results. XSS J00564+4548 exhibits a period of 465.68 - 0.07 s, which we interpret as the spin period, an energy dependent modulation depth, and a spectrum that is fit by a 22 keV photoelectrically absorbed bremsstrahlung with an iron line profile. IGR J17195-4100 shows several candidate periodicities and a spectrum that is fit by a power law with an iron line. XSS J12270-4859 exhibits a candidate spin period of 859.57 0.64 s and a spectrum that is fit by a power law with no evidence of an iron line.Conclusions. XSS J00564+4548 is confirmed to be an intermediate polar. IGR J17195-4100 and XSS J12270-4859 both show some properties of intermediate polars, but cannot be confirmed as definite members of the class here. © 2008 ESO.
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Butters, O. W., Norton, A. J., Hakala, P., Mukai, K., & Barlow, E. J. (2008). RXTE determination of the intermediate polar status of XSS J00564+4548, IGR J17195-4100, and XSS J12270-4859. Astronomy and Astrophysics, 487(1), 271–276. https://doi.org/10.1051/0004-6361:200809942
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