TY - JOUR
T1 - Peculiar spin frequency and radio profile evolution of PSR J1119-6127 following magnetar-like X-ray bursts
AU - Dai, S.
AU - Johnston, S.
AU - Weltevrede, P.
AU - Kerr, M.
AU - Burgay, M.
AU - Esposito, P.
AU - Israel, G.
AU - Possenti, A.
AU - Rea, N.
AU - Sarkissian, J.
PY - 2018
Y1 - 2018
N2 - We present the spin frequency and profile evolution of the radio pulsar J1119-6127 following magnetar-like X-ray bursts from the system in 2016 July. Using data from the Parkes radio telescope, we observe a smooth and fast spin-down process subsequent to the X-ray bursts resulting in a net change in the pulsar rotational frequency of Δv ≈-4 ÃÂ 10-4 Hz. During the transition, a net spin-down rate increase of Δ v ≈ -1 ÃÂ 10-10 Hz s-1 is observed, followed by a return of v to its original value. In addition, the radio pulsations disappeared after the X-ray bursts and reappeared about two weeks later with the flux density at 1.4 GHz increased by a factor of 5. The flux density then decreased and undershot the normal flux density followed by a slow recovery back to normal. The pulsar's integrated profile underwent dramatic and short-term changes in total intensity, polarization, and position angle. Despite the complex evolution, we observe correlations between the spin-down rate, pulse profile shape, and radio flux density. Strong single pulses have been detected after the X-ray bursts with their energy distributions evolving with time. The peculiar but smooth spin frequency evolution of PSR J1119-6127 accompanied by systematic pulse profile and flux density changes aremost likely to be a result of either reconfiguration of the surface magnetic fields or particle winds triggered by the X-ray bursts. The recovery of spin-down rate and pulse profile to normal provides us the best case to study the connection between high magnetic-field pulsars and magnetars.
AB - We present the spin frequency and profile evolution of the radio pulsar J1119-6127 following magnetar-like X-ray bursts from the system in 2016 July. Using data from the Parkes radio telescope, we observe a smooth and fast spin-down process subsequent to the X-ray bursts resulting in a net change in the pulsar rotational frequency of Δv ≈-4 ÃÂ 10-4 Hz. During the transition, a net spin-down rate increase of Δ v ≈ -1 ÃÂ 10-10 Hz s-1 is observed, followed by a return of v to its original value. In addition, the radio pulsations disappeared after the X-ray bursts and reappeared about two weeks later with the flux density at 1.4 GHz increased by a factor of 5. The flux density then decreased and undershot the normal flux density followed by a slow recovery back to normal. The pulsar's integrated profile underwent dramatic and short-term changes in total intensity, polarization, and position angle. Despite the complex evolution, we observe correlations between the spin-down rate, pulse profile shape, and radio flux density. Strong single pulses have been detected after the X-ray bursts with their energy distributions evolving with time. The peculiar but smooth spin frequency evolution of PSR J1119-6127 accompanied by systematic pulse profile and flux density changes aremost likely to be a result of either reconfiguration of the surface magnetic fields or particle winds triggered by the X-ray bursts. The recovery of spin-down rate and pulse profile to normal provides us the best case to study the connection between high magnetic-field pulsars and magnetars.
UR - https://hdl.handle.net/1959.7/uws:63823
U2 - 10.1093/MNRAS/STY2063
DO - 10.1093/MNRAS/STY2063
M3 - Article
SN - 0035-8711
VL - 480
SP - 3584
EP - 3594
JO - Monthly Notices of the Royal Astronomical Society
JF - Monthly Notices of the Royal Astronomical Society
IS - 3
ER -