
1.
Gamma-Ray Pulsar Visibility - Venter, C.; de Jager, O. C.; Tiplady, A. PSR J0437-4715 is a millisecond pulsar (MSP) thought to be ``pair formationstarved'' (having limited pair cascades due to magnetic photon absorption).

2.
Electrodynamics of pulsar magnetospheres - Spitkovsky, Anatoly I review the theoretical understanding of the global structure of pulsarmagnetospheres concentrating on recent progress in force-free electrodynamicsand first-principles simulations of magnetospheres.

3.
Radio pulsar death - Zhang, Bing Pulsar radio emission is believed to be originated from the electron-positronpairs streaming out from the polar cap region.

4.
Revised Pulsar Spindown - Contopoulos, Ioannis; Spitkovsky, Anatoly We address the issue of electromagnetic pulsar spindown by combining ourexperience from the two limiting idealized cases which have been studied ingreat extent in the past: that of an aligned rotator where ideal MHD conditionsapply, and that of a misaligned rotator in vacuum.

5.
Reviewing Pulsar Spectra - Sieber, W. Pulsar research must be considered - 35 years after thedetection of pulsars - a mature science, where the basic questions have beenraised and discussed.

6.
Power of a Turbulent Pulsar - Gruzinov, Andrei The turbulent jet entrains poloidal flux as it propagates awayfrom the star.

7.
Pulsar virtual observatory - Keith, M.; Harbulot, B.; Lyne, A.; Brooke, J. The Pulsar Virtual Observatory will provide a means for scientists in allfields to access and analyze the large data sets stored in pulsar surveyswithout specific knowledge about the data or the processing mechanisms.

8.
On "Pulsar dynamics: magnetic dipole model revisited" - Barsukov, D. P.; Kantor, E. M.; Tsygan, A. I. Comments on the article "Pulsar dynamics: magnetic dipole model revisited".

9.
Pulsar Luminosity Function - Guseinov, O. H.; Yazgan, E.; Ozkan, S.; Tagieva, S. We construct and investigate the pulsar luminosity function using the newcatalogue which includes data for 1315 radio pulsars.

10.
Pulsar Signal of Deconfinement - Glendenning, Norman K. A solitary millisecond pulsar, if near the mass limit, and undergoing a phasetransition, either first or second order, provided the transition is to asubstantially more compressible phase, will emit a blatantly obvioussignal---spontaneous spin-up.

11.
Dissipation in Pulsar Winds - Kirk, J. G. I review the constraints placed on relativistic pulsar winds by comparingoptical and X-ray images of the inner Crab Nebula on the one hand withtwo-dimensional MHD simulations on the other.

12.
The Vela pulsar, the key? - Dodson, Richard; Lewis, Dion; Legge, David; McCulloch, Peter; Reynolds, John; McConnell, David; Deshpande, Avinash Of all pulsars known Vela has been one of the most productive in terms inunderstanding pulsars and their characteristics.

13.
On the Pulsar Emission Mechanism - Cea, Paolo We discuss a general mechanism which allows to explain naturally both radioand high energy emission by pulsars.

14.
Electromagnetic pulsar spindown - Contopoulos, I. We evaluate the result of the recent pioneering numerical simulations inSpitkovsky~2006 on the spindown of an oblique relativistic magnetic dipolerotator.

15.
GCRT J1745-3009: A precessing radio pulsar? - Zhu, W. W.; Xu, R. X. This paper shows that most of theobserved features can be reproduced by our proposed precessing pulsar model.

16.
Fitting Pulsar Wind Tori - Ng, C. -Y.; Romani, Roger W. CXO imaging has shown that equatorial tori, often with polar jets, are verycommon in young pulsar wind nebulae (PWNe).

17.
Pulsar Braking Indices Revisited - Johnston, Simon; Galloway, David Using the standard equation for the slowdown of a neutron star, we derive aformula for the braking index via integration rather than the conventionaldifferentiation.

18.
Pulsar: repeatable Lagrangian singularity - Chigirinsky, Alexander V. In general, the interior of radially symmetric self-gravitating sphere isconsidered in terms of hydrostatic equilibrium (HSE).

19.
Modeling Pulsar Wind Nebulae - Bucciantini, N. In the last few years, new observations by CHANDRA and XMM have shown thatPulsar Wind Nebulae present a complex but similar inner feature, with thepresence of axisymmetric rings and jets, which is generally referred as {\itjet-torus structure}.

20.
Radio Pulsar Timing - Bell, J. F. The motivation for radio pulsar timing and its basic principles are reviewed.