Volume 498, Number 2, May I 2009
|Page(s)||L17 - L19|
|Published online||27 March 2009|
Letter to the Editor
RXTE confirmation of the intermediate polar status of IGR J15094–6649
Department of Physics and Astronomy, University of Leicester, Leicester LE1 7RH, UK e-mail: firstname.lastname@example.org
2 Department of Physics and Astronomy, The Open University, Walton Hall, Milton Keynes MK7 6AA, UK
3 CRESST and X-ray Astrophysics Laboratory NASA/GSFC, Greenbelt, MD 20771, USA
4 Department of Physics, University of Maryland, Baltimore County, 1000 Hilltop Circle, Baltimore, MD 21250, USA
Accepted: 13 March 2009
Aims. We aim to establish the X-ray properties of the intermediate polar candidate IGR J15094–6649 and therefore confirm its inclusion into the class.
Methods. 42 856 s of X-ray data from RXTE was analysed. Frequency analysis was used to constrain temporal variations and spectral analysis used to characterise the emission and absorption properties.
Results. A spin period of 809.7 ± 0.6 s is present, revealed as a complex pulse profile whose modulation depth decreases with increasing X-ray energy. The spectrum is well fitted by either a 17 ± 4 keV Bremsstrahlung or Γ = 1.8 ± 0.1 power law, with an iron emission line feature and significant absorption in each case.
Conclusions. IGR J15094–6649 is confirmed to be an intermediate polar.
Key words: stars: binaries: general / stars: novae, cataclysmic variables / stars: individual: IGR J15094-6649 / X-rays: binaries
© ESO, 2009
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