11 citations · 11 across the 2 of their papers we have counts for
5 papers · 1 filter
The Large-Scale Magnetic Field Structure of Our Galaxy: Efficiently Deduced from Pulsar Rotation Measures
J. L. Han
In this review, I will first introduce possible methods to probe the large-scale magnetic fields in our Galaxy and discuss their limitations. The magnetic fields in the Galactic ha…
Searching for sub-millisecond pulsars from highly polarized radio sources
J. L. Han, R. N. Manchester, A. G. Lyne +1
Pulsars are among the most highly polarized sources in the universe. The NVSS has catalogued 2 million radio sources with linear polarization measurements, from which we have selec…
Possible re-acceleration regions above the inner gap and pulsar gamma-ray emission
B. H. Hong, G. J. Qiao, B. Zhang +2
We propose that the violent breakdown of the Ruderman-Sutherland type vacuum gap above the pulsar polar cap region may produce copious primary particles and make the charge density…
Polarization Characteristics of Pulsar Profiles
J. L. Han, R. N. Manchester, G. J. Qiao
Polarization profiles of several hundred pulsars have been published recently (eg. Gould & Lyne 1998, GL98; Weisberg et al. 1999). In this report, we summarize the characteristics…
New clues to the magnetic field structure of M31
J. L. Han, R. Beck, E. M. Berkhuijsen
We observed 21 polarized background radio sources in the field of M31 at 1.365 GHz and 1.652 GHz, and determined their rotation measures (RMs). The RM data show that the regular ma…