High-energy Phase-averaged Spectra From Vela and PSR B1951+32

摘要：

We study high-energy radiation properties based on the vacuum outer gap model given by Zhang et al. (2004). The trans-field height (or fractional size) and the radii of inner and outer boundaries of the outer gap can be determined for a pulsar with a known magnetic inclination angle. Then, the radiation along the Κ th field lines is treated as a typical high-energy radiation, we calculate highenergy spectra for Vela and PSR B1951+32.

关键词： gamma-ray theory - pulsars general - radiation mechanisms nonther-mal - stars magnetic fields

作者: Y. Meng L. Zhang Z. J. Jiang

作者单位: Department of Physics, Yunnan University , Kunming, China

会议类型: 国际会议

会议名称: The 10th Asian-Pacific Regional International Astronomical Union Meeting(第十届亚洲及太平洋地区天文学大会 APRIM)

会议地点: 昆明

会议语种:英文

页码: 244-245

在线出版日期: 2008-08-03（万方平台首次上网日期，不代表论文的发表时间）