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

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

Internet

http://purl.org/au-research/grants/arc/FT140101082
http://hdl.handle.net/20.500.11937/80101

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