Studies of the gamma ray pulsar Geminga

被引：0

作者：

Zhang, S ^{[1
]}

Li, TP ^{[1
]}

Wu, M ^{[1
]}

Yu, W ^{[1
]}

Sun, XJ ^{[1
]}

Song, LM ^{[1
]}

Lu, FJ ^{[1
]}

机构：

[1] Inst High Energy Phys, High Energy Astrophys Lab, Beijing 100039, Peoples R China

来源：

PROCEEDINGS OF THE FOURTH COMPTON SYMPOSIUM, PTS 1 AND 2: PT 1: THE COMPTON OBSERVATORY IN REVIEW; PT 2: PAPERS AND PRESENTATIONS | 1997年 / 410期

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Ephemeris parameters of gamma ray pulsar Geminga have been revised using EGRET. Timing and imaging analyses show that the majority emission of Geminga are in phase region around the first peak in 10-30 MeV during COMPTEL VP1. No turn off of spectrum appear at energies below 30 MeV.

引用

页码：578 / 582

页数：5

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