The very faint X-ray binary IGR J17062-6143: a truncated disc, no pulsations, and a possible outflow

The very faint X-ray binary IGR J17062-6143: a truncated disc, no pulsations, and a possible outflow

We present a comprehensive X-ray study of the neutron star low-mass X-ray binary IGR J17062-6143, which has been accreting at low luminosities since its discovery in 2006. Analysing NuSTAR, XMM-Newton, and Swift observations, we investigate the very faint nature of this source through three approach...

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Bibliographic Details
Main Authors: van den Eijnden, J (Author), Degenaar, N (Author), Pinto, C (Author), Patruno, A (Author), Wette, K (Author), Messenger, C (Author), Hernández Santisteban, J V (Author), Wijnands, R (Author), Miller, J M (Author), Altamirano, D (Author), Paerels, F (Author), Fabian, A C (Author), Chakrabarty, Deepto (Contributor)
Other Authors: Massachusetts Institute of Technology. Department of Physics (Contributor)
Format: Article
Language:English
Published: Oxford University Press (OUP), 2019-03-15T12:48:21Z.
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