星射线

并结合技术框架给出了脉冲星X射线脉冲星姿态测量的工作流程。

The process of Attitude measurement based on X-ray Pulsar is given with the technology frameworks .

多柔比星X射线联合诱导大鼠C6胶质瘤细胞凋亡

Synergistic Induction of Apoptosis by Adriamycin and X Radiation in Rat C6 Glioma

方法：通过光镜、电镜、DNA断裂分析，进行多柔比星X射线联合诱导C6胶质瘤细胞凋亡研究。

Methods Rat C6 glioma cell line was exposed in vitro to adriamycin assisted with X radiation . Cell apoptosis was ascertained by cell morphology and DNA fragment analysis study .

广义相对论效应对脉冲星γ射线辐射的影响

Influence of general relativistic effects on γ - ray radiation from Pulsars

本文作者在脉冲星γ射线辐射的极冠模型的基础上，考虑光子在磁层中的级联过程，提出了级联过程中能量转化效率的概念并得出了转化效率公式。

Based on the polar cap model of pulsar γ - ray emission , considering the cascade process of photon in the magnetosphere , we propose the concept of transposition efficiency of energy in the cascade process and obtain the formula of it in this paper .

类太阳活动星的X射线观测与研究进展

Progress in the X-ray Observation and Study of Solar Like Stars

脉冲星、X射线双星以及γ射线爆源，都可能存在着这种第二类磁场。

Its properties implied from pulsars , X-ray binaries and gamma-ray bursts are discussed .

孤立脉冲星的X射线光度

X - Ray Luminosity of Isolated Pulsars

根据RS模型，给出了脉冲星的γ射线辐射机制，并简单地讨论了六个已发现的γ射线脉冲星。

Based on Ruderman-Sutherland model , pulsars emission mechanisms are given here aiid six γ - rag pulsars are dix-cussed briefly .

据XPNAV-1卫星研究项目首席科学家帅平表示，这颗卫星的主要目的是要检测地球附近26颗脉冲星的X射线信号详细信息，建立一个“脉冲导航数据库”。

According to Shuai Ping , chief scientist behind the research of XPNAV-1 satellite , the key aim of this satellite is to detect the details of X-ray signals of 26 nearby pulsars , and to create a " pulsar navigation database . "

用中心有脉冲星的γ射线暴的火球模型计算出GRB970228和GRB000301c两个γ射线暴的余辉辐射流，计算结果与观测结果相比较，符合的很好。

The radiation flux of two gamma-ray bursts ( GRB970228 and GRB000301 ) afterglows has been studied using the fireball model with a millisecond pulsar at the center , which turns out to be well consistent with the observation data .

偶极和四极磁场下脉冲星的γ射线辐射

γ - ram pulsars emission existing dipole and quadrupole magnetic fields

奇异星与γ射线暴的能源机制

A Strange Star and Energy Mechanisms of γ - ray Bursts

第四章介绍目前主要的Be单星和Be/X射线双星模型；

The fourth introduces the main models of Be stars and Be / X-ray binaries ;

一旦进入轨道，该望远镜将被用于观测诸如黑洞、脉冲星和伽马射线暴等高能实体，以更好地理解它们的能量来源。

Once in orbit , the telescope will be used to observe high-energy entities like black holes , pulsars and gamma-ray bursts in order to understand more about their energy sources .

星载核爆X射线探测技术进展天基核爆信号识别处理系统技术方案研究

Developments of nuclear explosion detection system on satellite A project of space-based detection for nuclear explosion

脉冲星B的X射线辐射能够被看到可能是因为脉冲星A的星风阻断了脉冲星B的磁层，为脉冲星B的星风提供了动力并加热中子星的表面。

Pulsar B 's X-ray emission might be visible because pulsar A 's wind intercepts the magnetosphere of pulsar B , powering pulsar B 's wind and heating up the neutron star 's surface .

蟹状星云脉冲星的TeVγ射线周期发射

Pulsed Emission of Very High Energy Gamma-Rays From Crab Pulsar