A re-establishing jet during an X-ray re-brightening of the Be/X-ray binary Swift J0243.6+6124

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A re-establishing jet during an X-ray re-brightening of the Be/X-ray binary Swift J0243.6+6124

© 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. Transient Be/X-ray binary systems, wherein a compact object accretes from a Be-companion star, can show giant and periastron outbursts. During the decay of their giant outbursts, some Be/X-ray bin...

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Bibliographic Details
Main Authors:	Van Den Eijnden, J., Degenaar, N., Russell, T.D., Hernández Santisteban, J.V., Wijnands, R., Miller-Jones, James, Rouco Escorial, A., Sivakoff, G.R.
Format:	Journal Article
Language:	English
Published:	OXFORD UNIV PRESS 2019
Subjects:	Science & Technology Physical Sciences Astronomy & Astrophysics accretion, accretion discs stars: neutron pulsars: individual: Swift J0243.6+6124 X-rays: binaries DISC INSTABILITY MODEL NEUTRON-STAR MAGNETIC-FIELD RADIO-EMISSION SAX J1808.4-3658 LOW/HARD STATE STELLAR WIND DWARF NOVAE ACCRETION PULSAR
Online Access:	http://purl.org/au-research/grants/arc/FT140101082 http://hdl.handle.net/20.500.11937/80101

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