The Radio-loud Magnetar PSR J1622-4950

Details The Radio-loud Magnetar PSR J1622-4950 The Radio-loud Magnetar PSR J1622-4950

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aipc.1357..177l&link_type=abstract

RADIO PULSARS: AN ASTROPHYSICAL KEY TO UNLOCK THE SECRETS OF THE UNIVERSE. AIP Conference Proceedings, Volume 1357, pp. 177-180

Other

Radio, Pulsars, Magnetic Fields, Neutron Stars, Radio, Microwave, Pulsations, Oscillations, And Stellar Seismology, Electric And Magnetic Fields, Neutron Stars

Scientific paper

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.

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