We re-examine the evidence for alignment of the proper motion and fiducial polarization-angle directions in radio pulsars given by Johnston et al., and we find that the case is probably stronger than this paper asserts. Other alignments are examined using the published literature and recent Arecibo polarimetry, providing an enlarged case that pulsar rotation axis and supernovae ``kick'' directions are aligned or orthogonal at birth. Pulsars' ``orthogonal'' polarization modes complicate fixing the orientation of such ``kicks,'' but we note that determining the absolute geometry of the polarization modes is a key objective for understanding the physical origins of pulsar emission
The comparison of the orientations of the optical-polarization vectors of quasars that are separated...
In an earlier paper we introduced a model for pulsars in which nonradial oscillations of high spheri...
The circular polarization associated with pulsar emission is examined phenomenologically. Virtually ...
We present strong observational evidence for a relationship between the direction of a pulsar's moti...
We review our case for strong observational evidence for a relationship between the direction of a p...
We have conducted observations of 22 pulsars at frequencies of 0.7, 1.4 and 3.1 GHz and present thei...
Restricted Access.An elegant mechanism to explain the high velocities of pulsars has been proposed b...
We present here a direct comparison of the polarization position angle (PA) profiles of 17 pulsars, ...
The observed polarisation angle variation in pulsars is analysed on the basis of the magnetic pole m...
We present here a direct comparison of the polarisation position angle (PA) profiles of 17 pulsars, ...
Polarization observations of the radio emission from PSR B2016+28 at 1404 MHz reveal properties that...
Polarization is one of the striking characteristies of pulsar's emission. The integrated profil...
We study implications for the apparent alignment of the spin axes, proper motion directions, and pol...
Despite some success in explaining the observed polarization angle swing of radio pulsars within the...
We report here the discovery of a significant source of systematic error in the rotation measure det...
The comparison of the orientations of the optical-polarization vectors of quasars that are separated...
In an earlier paper we introduced a model for pulsars in which nonradial oscillations of high spheri...
The circular polarization associated with pulsar emission is examined phenomenologically. Virtually ...
We present strong observational evidence for a relationship between the direction of a pulsar's moti...
We review our case for strong observational evidence for a relationship between the direction of a p...
We have conducted observations of 22 pulsars at frequencies of 0.7, 1.4 and 3.1 GHz and present thei...
Restricted Access.An elegant mechanism to explain the high velocities of pulsars has been proposed b...
We present here a direct comparison of the polarization position angle (PA) profiles of 17 pulsars, ...
The observed polarisation angle variation in pulsars is analysed on the basis of the magnetic pole m...
We present here a direct comparison of the polarisation position angle (PA) profiles of 17 pulsars, ...
Polarization observations of the radio emission from PSR B2016+28 at 1404 MHz reveal properties that...
Polarization is one of the striking characteristies of pulsar's emission. The integrated profil...
We study implications for the apparent alignment of the spin axes, proper motion directions, and pol...
Despite some success in explaining the observed polarization angle swing of radio pulsars within the...
We report here the discovery of a significant source of systematic error in the rotation measure det...
The comparison of the orientations of the optical-polarization vectors of quasars that are separated...
In an earlier paper we introduced a model for pulsars in which nonradial oscillations of high spheri...
The circular polarization associated with pulsar emission is examined phenomenologically. Virtually ...