FLARES IN THE X-RAY SOURCE EXO-2030 + 375

被引：8

作者：

APPARAO, KMV

机构：

[1] Department of Astronomy, Pennsylvania State University, University Park

[2] Tata Inst. of Fundamental Research, Bombay

来源：

ASTROPHYSICAL JOURNAL | 1991年 / 375卷 / 02期

关键词：

STARS; BE; INDIVIDUAL; (EXO-2030; 375); X-RAYS; BINARIES; BURSTS;

D O I：

10.1086/170235

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Six X-ray flares were observed in the source EXO 2030 + 375 with an average time interval of about 4 hr between the flares. It is shown here that the flares can be due to Rayleigh-Taylor instabilities near the magnetospheric boundary of the neutron star when it reaches the equilibrium period.

引用

页码：701 / 703

页数：3

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