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QPO in RE J1034+396: model constraints from observed trends

We analyze the time variability of the X-ray emission of RE J1034+396, an active galactic nucleus with the first firm detection of a quasi-periodic oscillations (QPO). Based on the results of a wavelet analysis, we find a drift in the QPO central frequency. The change inthe QPO frequency correlates with the change in the X-ray flux with a short time delay. Linear structures such as shocks, spiral waves, orvery distant flares seem to be a favored explanation for this particular QPO event.

preprint2012arXivOpen access
B. CzernyP. LachowiczM. DovciakV. KarasT. PechacekTapas K. Das
astro-ph.COastro-ph.HE
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Open access6 authors2 topics
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B. CzernyP. LachowiczM. DovciakV. KarasT. PechacekTapas K. Das

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