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, Degenaar, N, Pinto, C, Patruno, A, Wette, K, Messenger, C, Hernández Santisteban, J V, Wijnands, R, Miller, J M, Altamirano, D, Paerels, F, Fabian, A C, Chakrabarty, Deepto
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Published: Oxford University Press (OUP) 2019
Online Access:http://hdl.handle.net/1721.1/120975
https://orcid.org/0000-0001-8804-8946

Internet

http://hdl.handle.net/1721.1/120975
https://orcid.org/0000-0001-8804-8946

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