The low luminosity behaviour of the 4U 0115+63 Be/X-ray transient

Alessandro Patruno; Alicia Rouco Escorial; Ann-Sofie Bak Nielsen; Nathalie Degenaar; Rudy Wijnands; Yuri Cavecchi

The low luminosity behaviour of the 4U 0115+63 Be/X-ray transient

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arxiv 1704.00284 v2 pith:5XFQM6DY submitted 2017-04-02 astro-ph.HE

Alicia Rouco Escorial , Ann-Sofie Bak Nielsen , Rudy Wijnands , Yuri Cavecchi , Nathalie Degenaar , Alessandro Patruno This is my paper · ORCID

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The Be/X-ray transient 4U 0115+63 exhibited a giant, type-II outburst in October 2015. The source did not decay to its quiescent state but settled in a meta-stable plateau state (a factor ~10 brighter than quiescence) in which its luminosity slowly decayed. We used XMM-Newton to observe the system during this phase and we found that its spectrum can be well described using a black-body model with a small emitting radius. This suggests emission from hot spots on the surface, which is confirmed by the detection of pulsations. In addition, we obtained a relatively long (~7.9 ksec) Swift/XRT observation ~35 days after our XMM-Newton one. We found that the source luminosity was significantly higher and, although the spectrum could be fitted with a black-body model the temperature was higher and the emitting radius smaller. Several weeks later the system started a sequence of type-I accretion outbursts. In between those outbursts, the source was marginally detected with a luminosity consistent with its quiescent level. We discuss our results in the context of the three proposed scenarios (accretion down to the magnestospheric boundary, direct accretion onto neutron star magnetic poles or cooling of the neutron star crust) to explain the plateau phase.

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