SEARCH FOR HIGH ENERGY GAMMA-RAYS FROM CP 1133

被引：17

作者：

CHARMAN, WN

JELLEY, JV

ORMAN, PR

DREVER, RWP

MCBREEN, B

机构：

[1] Atomic Energy Research Establishment, Harwell

[2] Physics Department, University College

来源：

NATURE | 1968年 / 220卷 / 5167期

关键词：

D O I：

10.1038/220565a0

中图分类号：

O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];

学科分类号：

07 ; 0710 ; 09 ;

摘要：

SEVERAL proposed models for pulsars, involving shock waves1 and high magnetic fields2,3, suggest the possibility that high energy γ-rays may be emitted by such objects. We have therefore attempted to detect high energy (∼ 1014 eV), neutral cosmic rays from CP 1133, using the atmospheric Cherenkov technique4. © 1968 Nature Publishing Group.

引用

页码：565 / &

共 12 条

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