Add to ORKGWe investigate the evolution of rotation period and spindown age of a pulsar whose surface magnetic field undergoes a phase of growth. Application of these results to the Crab pulsar strongly indicates that its parameters cannot be accounted for by the field growth theories
We have investigated the turbulent mean-field dynamo action in protoneutron stars that are subject ...
We investigate the time-dependent behaviour of Crab-like pulsar wind nebulae (PWNe) generating a set...
Statistical analysis has been carried out of the relations between period and the age P - t(c), and ...
We investigate the evolution of rotation period and spindown age of a pulsar whose surface magnetic ...
The evolution of rotation period and spindown age of a pulsar whose surface magnetic field undergoes...
The evolutions of a neutron star's rotation and magnetic field (B-field) have remained unsolved puzz...
In the standard scenario for spin evolution of isolated neutron stars, a young pulsar slows down wit...
Magnetic dissipation is frequently invoked as a way of powering the observed emission of relativisti...
Pulsars are highly magnetized and rapidly rotating neutron stars. The magnetic field can reach the c...
accepted for publication in Astronomy & AstrophysicsNew results based on methods of population synth...
Radio pulsars are thought to spin down primarily as a result of torque from magnetic dipole radiatio...
The Crab pulsar has suffered in 1975 and 1989 two glitches in which the frequency did not relaxed to...
The pattern of glitches and postglitch behavior observed for the Crab pulsar (Boynton et al. 1972; D...
Is pulsar make up of strange matter? The magnetic field decay of a pulsar may be able to give us an ...
We use a modified pulsar current analysis to study magnetic field decay in radio pulsars. In our app...
We have investigated the turbulent mean-field dynamo action in protoneutron stars that are subject ...
We investigate the time-dependent behaviour of Crab-like pulsar wind nebulae (PWNe) generating a set...
Statistical analysis has been carried out of the relations between period and the age P - t(c), and ...
We investigate the evolution of rotation period and spindown age of a pulsar whose surface magnetic ...
The evolution of rotation period and spindown age of a pulsar whose surface magnetic field undergoes...
The evolutions of a neutron star's rotation and magnetic field (B-field) have remained unsolved puzz...
In the standard scenario for spin evolution of isolated neutron stars, a young pulsar slows down wit...
Magnetic dissipation is frequently invoked as a way of powering the observed emission of relativisti...
Pulsars are highly magnetized and rapidly rotating neutron stars. The magnetic field can reach the c...
accepted for publication in Astronomy & AstrophysicsNew results based on methods of population synth...
Radio pulsars are thought to spin down primarily as a result of torque from magnetic dipole radiatio...
The Crab pulsar has suffered in 1975 and 1989 two glitches in which the frequency did not relaxed to...
The pattern of glitches and postglitch behavior observed for the Crab pulsar (Boynton et al. 1972; D...
Is pulsar make up of strange matter? The magnetic field decay of a pulsar may be able to give us an ...
We use a modified pulsar current analysis to study magnetic field decay in radio pulsars. In our app...
We have investigated the turbulent mean-field dynamo action in protoneutron stars that are subject ...
We investigate the time-dependent behaviour of Crab-like pulsar wind nebulae (PWNe) generating a set...
Statistical analysis has been carried out of the relations between period and the age P - t(c), and ...