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arXiv · 1905.05773

Peculiar outbursts of an ultra luminous source likely signs of an aperiodic disc-wind

H. Stiele·A. K. H. Kong
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Abstract

The metal rich globular cluster RZ 2109 in the massive Virgo elliptical galaxy NGC 4472 (M49) harbours the ultra luminous X-ray source XMMU 122939.7+075333. Previous studies showed that this source varies between bright and faint phases on timescales of just a few hours. Here, we report the discovery of two peculiar X-ray bursting events that last for about 8 and 3.5 hours separated by about 3 days. Such a recurring X-ray burst-like behaviour has never been observed before. We argue that type-I X-ray bursts or super bursts as well as outburst scenarios requiring a young stellar object are highly unlikely explanations for the observed light curve, leaving an aperiodic disc wind scenario driven by hyper-Eddington accretion as a viable explanation for this new type of X-ray flaring activities.

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H. Stiele, A. K. H. Kong. 2019-05-14. Peculiar outbursts of an ultra luminous source likely signs of an aperiodic disc-wind. https://doi.org/10.3847/1538-4357%2Fab1e4b

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