标题： 毫秒脉冲星伽马射线发射的宽频模型谱 显示英文标题

标题： Broad-Band Model Spectra of Gamma-Ray Emission from Millisecond Pulsars

摘要： 我们提出了在极帽模型框架下预计来自毫秒脉冲星的脉冲伽马射线辐射谱。这些谱是由曲率辐射（CR）、同步辐射（SR）和康普顿上散射（ICS）三种成分叠加而成。CR 成分在低于$100 $GeV 时占主导地位，而 ICS 成分在$\sim 1 $太电子伏特处显示出峰值。CR 成分应该能够通过下一代伽马射线望远镜（例如 GLAST）从 J0437-4715 中观测到。 显示英文摘要

摘要： We present spectra of pulsed gamma-ray emission expected from millisecond pulsars within the framework of polar-cap models. The spectra are a superposition of three components due to curvature (CR), synchrotron (SR), and Compton upscattering (ICS) processes. The CR component dominates below $100 $GeV and the ICS component exhibits a peak at $\sim 1 $TeV. The CR component should be observable from J0437-4715 with the next generation gamma-ray telescopes, like e.g. GLAST.