RXTE confirmation of the intermediate polar status of IGR J15094-6649
Abstract
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.
- Publication:
-
Astronomy and Astrophysics
- Pub Date:
- May 2009
- DOI:
- arXiv:
- arXiv:0901.3983
- Bibcode:
- 2009A&A...498L..17B
- Keywords:
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- stars: binaries: general;
- stars: novae;
- cataclysmic variables;
- stars:;
- individual: IGR J15094-6649;
- X-rays: binaries;
- Astrophysics - Solar and Stellar Astrophysics;
- Astrophysics - High Energy Astrophysical Phenomena
- E-Print:
- 3 pages, 5 figures. Submitted to A&