We investigate the spin evolution of the binary X-ray pulsar 2S 0114+650, which possesses the slowest known spin period of $\sim 2.7$ hours. We argue that, to interpret such long spin period, the magnetic field strength of this pulsar must be initially $\gsim 10^{14}$ G, that is, it was born as a magnetar. Since the pulsar currently has a normal magnetic field $\sim 10^{12}$ G, our results present support for magnetic field decay predicted by the magnetar model
Recent measurements showed that the period derivative of the ‘hig h-B’ radio pulsar PSR J1734−3333 ...
Anomalous X-ray pulsars and soft gamma repeaters have recently emerged as a unified class of neutron...
The recurrent fast radio burst FRB 180916 was recently shown to exhibit a 16-d period (with possible...
Several relatively bright, persistent X-ray sources display regular pulses, with periods in the rang...
The X-ray source 1E 161348-5055 in the supernova remnant RCW 103 recently exhibited X-ray activity t...
2S 0114+650, GX 301-2, IGR J16358-4726, X Per, 4U 2206+54, SXP 1062, and 3A 1954+319 are thought to ...
The radio pulsar GLEAM-X J162759.5-523504.3 has an extremely long spin period ($P = 1091.17\, \mbox{...
We confront theoretical models for the rotational, magnetic, and thermal evolution of an ultra-magne...
Context. The recent discovery of long-period, low magnetic field pulsars in low-mass X-ray binaries ...
Magnetars are neutron stars in which a strong magnetic field is the main energy source. About two do...
PSR J1814-1744 is a 4 s radio pulsar with surface dipole magnetic field strength 5.5*10^13 G, inferr...
We present a population synthesis study of the observed properties of the magnetars investigating th...
Recent observations show that supergiant fast X-ray transients (SFXTs) spend most of their lifetime ...
Magnetars are young neutron stars with extreme magnetic fields (B ≳ 10^(14)-10^(15) G). How these fi...
The 6.67 hr periodicity and the variable X-ray flux of the central compact object (CCO) at the cente...
Recent measurements showed that the period derivative of the ‘hig h-B’ radio pulsar PSR J1734−3333 ...
Anomalous X-ray pulsars and soft gamma repeaters have recently emerged as a unified class of neutron...
The recurrent fast radio burst FRB 180916 was recently shown to exhibit a 16-d period (with possible...
Several relatively bright, persistent X-ray sources display regular pulses, with periods in the rang...
The X-ray source 1E 161348-5055 in the supernova remnant RCW 103 recently exhibited X-ray activity t...
2S 0114+650, GX 301-2, IGR J16358-4726, X Per, 4U 2206+54, SXP 1062, and 3A 1954+319 are thought to ...
The radio pulsar GLEAM-X J162759.5-523504.3 has an extremely long spin period ($P = 1091.17\, \mbox{...
We confront theoretical models for the rotational, magnetic, and thermal evolution of an ultra-magne...
Context. The recent discovery of long-period, low magnetic field pulsars in low-mass X-ray binaries ...
Magnetars are neutron stars in which a strong magnetic field is the main energy source. About two do...
PSR J1814-1744 is a 4 s radio pulsar with surface dipole magnetic field strength 5.5*10^13 G, inferr...
We present a population synthesis study of the observed properties of the magnetars investigating th...
Recent observations show that supergiant fast X-ray transients (SFXTs) spend most of their lifetime ...
Magnetars are young neutron stars with extreme magnetic fields (B ≳ 10^(14)-10^(15) G). How these fi...
The 6.67 hr periodicity and the variable X-ray flux of the central compact object (CCO) at the cente...
Recent measurements showed that the period derivative of the ‘hig h-B’ radio pulsar PSR J1734−3333 ...
Anomalous X-ray pulsars and soft gamma repeaters have recently emerged as a unified class of neutron...
The recurrent fast radio burst FRB 180916 was recently shown to exhibit a 16-d period (with possible...
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