Gamma-Ray Pulsars Expected in the Outer Gap Model of Gamma-Ray
Emission
ZHANG Li1,2, WU Jie2, JIANG Ze-Jun2, MEI Dong-Cheng2
1National Astronomical Observatories and Yunnan Observatory, Chinese Academy of Sciences, PO Box 110, Kunming 650010
2Department of Physics, Yunnan University, Kunming 650091
Gamma-Ray Pulsars Expected in the Outer Gap Model of Gamma-Ray
Emission
ZHANG Li1,2;WU Jie2;JIANG Ze-Jun2;MEI Dong-Cheng2
1National Astronomical Observatories and Yunnan Observatory, Chinese Academy of Sciences, PO Box 110, Kunming 650010
2Department of Physics, Yunnan University, Kunming 650091
Abstract： We study the possibility of high-energy gamma-ray emission from the known 1130 radio pulsars based on the outer gap model of high energy emission from pulsars. We estimate the fractional size of outer gap, the integrated flux, the gamma-ray luminosity for each known radio pulsar, and find that only 14% of the known radio pulsars are gamma-ray emitters according to the outer gap model. In the sample of possible 156 gamma-ray pulsars, our statistical analysis indicates that the distributions of the spin-down powers and the ages of these pulsars concentrate mainly on 1033.5-1039 erg/s and 103-107 y, respectively. The predictions of gamma-ray pulsars detected by the AGILE and GLAST missions are given.
ZHANG Li;WU Jie;JIANG Ze-Jun;MEI Dong-Cheng. Gamma-Ray Pulsars Expected in the Outer Gap Model of Gamma-Ray
Emission[J]. 中国物理快报, 2003, 20(3): 433-435.
ZHANG Li, WU Jie, JIANG Ze-Jun, MEI Dong-Cheng. Gamma-Ray Pulsars Expected in the Outer Gap Model of Gamma-Ray
Emission. Chin. Phys. Lett., 2003, 20(3): 433-435.
2003, Vol. 20 
