A strongly changing accretion morphology during the outburst decay of the neutron star X-ray binary 4U 1608−52
© 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...
Main Authors: | , , , , , , , , , |
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Format: | Article |
Language: | English |
Published: |
Oxford University Press (OUP)
2021
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Online Access: | https://hdl.handle.net/1721.1/135356 |