Swift-XRT Discovery of a 35s Periodicity in the 2006 Outburst of RS Ophiuchi

Astronomy and Astrophysics – Astronomy

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Scientific paper

The Swift-XRT discovered a 35 s oscillation in the soft X-ray emission from RS~Oph during the 2006 outburst. The modulation first appeared shortly after the start of the Super Soft Source phase (day 32.82) and remained visible until the soft X-ray emission began its decline (day 65.92), though it was absent at some times during this interval. In the initial stages the oscillation period was not stable and was multi-periodic at times. We suggest nuclear burning driven pulsations are the most likely cause of the oscillation.

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