Pulsed Radio Emission from PSR J1119-6127 disappeared

Open Access
Authors
Publication date 31-07-2016
Journal The astronomer's telegram
Volume | Issue number 9286
Organisations
  • Faculty of Science (FNWI) - Anton Pannekoek Institute for Astronomy (API)
  • Faculty of Science (FNWI)
Abstract We have searched for pulsed radio emission from the direction of the known high magnetic field pulsar PSR J1119-6127 (spin period of 409 ms, magnetic field intensity at surface of about 4 x 10^13 G, spin-down age of about 1700 yr, embedded in the supernova remnant SNR G292.2-0.5), which showed bursts similar to those typical of the Soft Gamma Repeaters (SGR) at 13:02:07.91 UT on 27 July 2016 (Younes et al,GCN Circular #19735) and at 01:27:51 UT on 28 July 2016 (Kennea et al,Atel #9274).
Document type Article
Language English
Published at http://www.astronomerstelegram.org/?read=9286
Other links https://ui.adsabs.harvard.edu/abs/2016ATel.9286....1B/abstract
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