most citedA Further Study of Relative longitude shift of Pulsar Beams

4 citations · 5 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2009

Statistics of Galactic Supernova Remnants (continued)

Jian-Wen Xu, Ya-Peng Hu

Our statistics on Galactic supernova remnants (SNRs) shows that the electrons temperature () of hard X-ray and the shock waves traveling velocity () decreases with age…

astro-ph.HE2009

A Unique Method to Determine SNe Initial Explosion Energy

Jian-Wen Xu, Hui-Rong Zhang

There are several different methods to determine the individual supernovae (SNe) initial explosion energy, here we derive the average or typical explosion energy of shell-type supe…

astro-ph.HE2009★ 1 cited

Distances to Two Galactic Supernova Remnants: G32.8-0.1 and G346.6-0.2

Jian-Wen Xu, Hui-Rong Zhang

There are either a near kinematic distance of 5.5 kpc or a far distance of 8.8 kpc for a Galactic supernova remnant (SNR) G32.80.1 derived by using the rotation curve of the Gal…

astro-ph.HE2009

Some Recent Progress on the Studies of Supernova Remnants

Jian-Wen Xu

We briefly reviewed some recent progress on the studies of supernova remnants (SNRs), including the radio SNRs (the structure, polarization, spectrum etc.), observational character…

astro-ph.HE2009

Theoretical Derivation of - Relation of Galactic SNRs

Jian-Wen Xu, Ya-Peng Hu, Hui-Rong Zhang

We derive the - relation of Galactic supernova remnants of shell-type separately at adiabatic-phase and at radiative-phase through two sets of different formulas, considering…

astro-ph2001★ 4 cited

A Further Study of Relative longitude shift of Pulsar Beams

R. X. Xu, J. W. Xu, G. J. Qiao

It is of great important to study pulsar beam shapes if we are concerned with emission theories and pulsar birth rate. Both observations and/or the inverse Compton scattering model…