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 ? = 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...
We have identified IGR J17303-0601 (1RXS J173021.5-055933) as an intermediate polar (IP). The optica...
Context. Based on XMM-Newton X-ray observations IGR J19552+0044 appears to be either a pre-polar or ...
We present the first optical photometry of the counterpart to the candidate intermediate polar RX J0...
Aims. We determine the nature of the intermediate polar candidates XSS J00564+4548 , IGR J17195-4100...
Aims. To determine the credentials of nine candidate intermediate polars in order to confirm whether...
Aims. We aim to establish the X-ray properties of the intermediate polar candidate IGR J15094–6649 a...
Aims. We aim to establish the X-ray properties of the intermediate polar candidate IGR J15094–6649 a...
Aims: We intend to establish the X-ray properties of Swift J0732.5-1331 and therefore confirm its st...
Aims. We aim to determine the credentials of nine candidate intermediate polars in order t...
Aims. We intend to establish the X-ray properties of Swift J0732.5–1331 and therefore confirm its st...
Aims. We intended to investigate the magnetic field properties of the recently identified intermedia...
Using X-ray observations from the NuSTAR and Swift satellites, we present temporal and spectral prop...
We have identified a new intermediate polar, HS 0943+1404, as part of our ongoing search for catacly...
Aims.We intend to establish the X-ray properties of Swift J0732.5–1331 and therefore confirm its st...
We present the results of our optical identification of the X-ray source IGR J16547-1916 detected by...
We have identified IGR J17303-0601 (1RXS J173021.5-055933) as an intermediate polar (IP). The optica...
Context. Based on XMM-Newton X-ray observations IGR J19552+0044 appears to be either a pre-polar or ...
We present the first optical photometry of the counterpart to the candidate intermediate polar RX J0...
Aims. We determine the nature of the intermediate polar candidates XSS J00564+4548 , IGR J17195-4100...
Aims. To determine the credentials of nine candidate intermediate polars in order to confirm whether...
Aims. We aim to establish the X-ray properties of the intermediate polar candidate IGR J15094–6649 a...
Aims. We aim to establish the X-ray properties of the intermediate polar candidate IGR J15094–6649 a...
Aims: We intend to establish the X-ray properties of Swift J0732.5-1331 and therefore confirm its st...
Aims. We aim to determine the credentials of nine candidate intermediate polars in order t...
Aims. We intend to establish the X-ray properties of Swift J0732.5–1331 and therefore confirm its st...
Aims. We intended to investigate the magnetic field properties of the recently identified intermedia...
Using X-ray observations from the NuSTAR and Swift satellites, we present temporal and spectral prop...
We have identified a new intermediate polar, HS 0943+1404, as part of our ongoing search for catacly...
Aims.We intend to establish the X-ray properties of Swift J0732.5–1331 and therefore confirm its st...
We present the results of our optical identification of the X-ray source IGR J16547-1916 detected by...
We have identified IGR J17303-0601 (1RXS J173021.5-055933) as an intermediate polar (IP). The optica...
Context. Based on XMM-Newton X-ray observations IGR J19552+0044 appears to be either a pre-polar or ...
We present the first optical photometry of the counterpart to the candidate intermediate polar RX J0...