A strongly changing accretion morphology during the outburst decay of the neutron star X-ray binary 4U 1608−52

A strongly changing accretion morphology during the outburst decay of the neutron star X-ray binary 4U 1608−52

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© 2020 The Author(s). It is commonly assumed that the properties and geometry of the accretion flow in transient lowmass X-ray binaries (LMXBs) significantly change when the X-ray luminosity decays below ∼10-2 of the Eddington limit (LEdd). However, there are few observational cases where the evolut...

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Bibliographic Details
Main Authors: van den Eijnden, J, Degenaar, N, Ludlam, RM, Parikh, AS, Miller, JM, Wijnands, R, Gendreau, KC, Arzoumanian, Z, Chakrabarty, D, Bult, P
Format: Article
Language:English
Published: Oxford University Press (OUP) 2021
Online Access:https://hdl.handle.net/1721.1/135356

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