The two known gamma ray pulsars, the Crab and Vela, were used as guides for the development of models of high-energy radiation from spinning neutron stars. Two general classes of models were developed: those with the gamma radiation originating in the pulsar magnetosphere far from the neutron star surface (outer gap models) and those with the gamma radiation coming from above the polar cap (polar cap models). The goal is to indicate how EGRET can contribute to understanding gamma-ray pulsars, and especially how it can help distinguish between models for emission
We have used a Monte Carlo simulation of a Polar Cap (PC) model of gamma-ray pulsars to estimate lig...
The reported e(sup +/-) annihilation line from the Crab pulsar has three remarkable properties. It i...
Information about the physical parameters of neutron stars is obtained from pulsar observations. The...
The advent of the next generation of gamma-ray experiments, led by GLAST, AGILE, INTEGRAL and a host...
The young pulsars in Crab and Vela were observed as very efficient emitters of high energy gamma rad...
We describe an emission model for gamma ray pulsars based on curvature radiation-reaction limited ch...
While the proposed research received partial funding under this grant, during the term of support su...
High-energy gamma rays are a valuable tool for studying particle acceleration and radiation in the m...
Pulsed emission from gamma-ray pulsars originates inside the magnetosphere, from radiation by charge...
We compute the variation of the beaming fraction with the efficiency of high energy fl-ray producti...
We have attempted to devise a scheme by which it may be possible to identify pulsars which are likel...
With the large sample of young gamma-ray pulsars discovered by the Fermi Large Area Telescope (LAT),...
Pulsars, a class of rotating neutron stars, are one of the most interesting objects of nature. Altho...
The Energetic Gamma-Ray Experiment Telescope (EGRET) on the Compton Gamma Ray Observatory has observ...
We consider high energy γ-ray radiation from the radio pulsars associated with some unidentified EGR...
We have used a Monte Carlo simulation of a Polar Cap (PC) model of gamma-ray pulsars to estimate lig...
The reported e(sup +/-) annihilation line from the Crab pulsar has three remarkable properties. It i...
Information about the physical parameters of neutron stars is obtained from pulsar observations. The...
The advent of the next generation of gamma-ray experiments, led by GLAST, AGILE, INTEGRAL and a host...
The young pulsars in Crab and Vela were observed as very efficient emitters of high energy gamma rad...
We describe an emission model for gamma ray pulsars based on curvature radiation-reaction limited ch...
While the proposed research received partial funding under this grant, during the term of support su...
High-energy gamma rays are a valuable tool for studying particle acceleration and radiation in the m...
Pulsed emission from gamma-ray pulsars originates inside the magnetosphere, from radiation by charge...
We compute the variation of the beaming fraction with the efficiency of high energy fl-ray producti...
We have attempted to devise a scheme by which it may be possible to identify pulsars which are likel...
With the large sample of young gamma-ray pulsars discovered by the Fermi Large Area Telescope (LAT),...
Pulsars, a class of rotating neutron stars, are one of the most interesting objects of nature. Altho...
The Energetic Gamma-Ray Experiment Telescope (EGRET) on the Compton Gamma Ray Observatory has observ...
We consider high energy γ-ray radiation from the radio pulsars associated with some unidentified EGR...
We have used a Monte Carlo simulation of a Polar Cap (PC) model of gamma-ray pulsars to estimate lig...
The reported e(sup +/-) annihilation line from the Crab pulsar has three remarkable properties. It i...
Information about the physical parameters of neutron stars is obtained from pulsar observations. The...