SAS-2 OBSERVATION OF PULSED HIGH-ENERGY GAMMA-RADIATION FROM GEMINGA

被引：36

作者：

MATTOX, JR ^{[1
]}

BERTSCH, DL ^{[1
]}

FICHTEL, CE ^{[1
]}

HARTMAN, RC ^{[1
]}

KNIFFEN, DA ^{[1
]}

THOMPSON, DJ ^{[1
]}

机构：

[1] HAMPDEN SYDNEY COLL,DEPT PHYS,HAMPDEN SYDNEY,VA 23943

来源：

ASTROPHYSICAL JOURNAL | 1992年 / 401卷 / 01期

关键词：

GAMMA-RAYS; OBSERVATIONS; PULSARS; INDIVIDUAL; (GEMINGA);

D O I：

10.1086/186661

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Following the detection of pulsed X-rays and gamma rays from Geminga, the 1972-1973 SAS 2 data which first revealed this source have been reanalyzed. The 237 ms periodicity is visible in those observations. The phase of the SAS 2 periodicity is consistent with that of COS B suggesting that the gamma-ray data allow an accounting for every revolution of the Geminga pulsar between 1972 and 1982.

引用

页码：L23 / L26

页数：4

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