Radio emission from the X-ray pulsar Her X-1: a jet launched by a strong magnetic field neutron star?
Her X-1 is an accreting neutron star (NS) in an intermediate-mass X-ray binary. Like lowmass X-ray binaries (LMXBs), it accretes via Roche lobe overflow, but similar to many high-mass X-ray binaries containing a NS; Her X-1 has a strong magnetic field and slow spin. Here, we present the discovery...
| Main Authors: | van den Eijnden, J., Degenaar, N., Russell, T., Miller-Jones, James, Wijnands, R., Miller, J., King, A., Rupen, M. |
|---|---|
| Format: | Journal Article |
| Published: |
Oxford University Press
2018
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| Online Access: | http://purl.org/au-research/grants/arc/FT140101082 http://hdl.handle.net/20.500.11937/69949 |
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