The radio-loud magnetar PSR J1622-4950
- Levin, L.
- Bailes, M.
- Bates, S. D.
- Bhat, N. D. R.
- Burgay, M.
- Burke-Spolaor, S.
- D'Amico, N.
- Johnston, S.
- Keith, M.
- Kramer, M.
- Milia, S.
- Possenti, A.
- Rea, N.
- Stappers, B.
- van Straten, W.
DOIAbstract
The High Time Resolution Universe survey for pulsars and fast transients has yielded the discovery of a slow radio pulsar, PSR J1622-4950, that despite its high dispersion measure exhibited a highly variable flux density and integrated pulse profile. The pulsar shares many properties with the two previously known magnetars that emit radio pulsations, including a similarly high inferred magnetic field strength. In contrast to other magnetars, PSR J1622-4950 shows no observed variations in X-ray emission
Add to ORKG