Disc-jet coupling in low-luminosity accreting neutron stars

Disc-jet coupling in low-luminosity accreting neutron stars

In outburst, neutron star X-ray binaries produce less powerful jets than black holes at a given X-ray luminosity. This has made them more difficult to study as they fade towards quiescence. To explore whether neutron stars power jets at low accretion rates (L X ? 10 36 erg s -1 ), we investigate t...

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Bibliographic Details
Main Authors: Tudor, V., Miller-Jones, James, Patruno, A., D'Angelo, C., Jonker, P., Russell, D., Russell, T., Bernardini, F., Lewis, F., Deller, A., Hessels, J., Migliari, S., Plotkin, Richard, Soria, Roberto, Wijnands, R.
Format: Journal Article
Published: Oxford University Press 2017
Online Access:http://purl.org/au-research/grants/arc/FT140101082
http://hdl.handle.net/20.500.11937/54333

Internet

http://purl.org/au-research/grants/arc/FT140101082
http://hdl.handle.net/20.500.11937/54333

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