THE CRUST SCREEN MODEL FOR THE MAGNETIC-FIELD OF BINARY-X-RAY SOURCES

CORC > 北京大学 > 地球与空间科学学院

	THE CRUST SCREEN MODEL FOR THE MAGNETIC-FIELD OF BINARY-X-RAY SOURCES
	ZHANG, CM ; WU, XJ ; YANG, GC
刊名	astronomy astrophysics
	1994
关键词	STAR, NEUTRON STARS, MAGNETIC FIELD X-RAYS, STARS STARS, BINARIES, CLOSE NEUTRON-STAR PULSAR DECAY ACCRETION EVOLUTION ORIGIN PERIOD
英文摘要	It is assumed that the compressed accretion matter on the crust of a neutron star with magnetic field has ferromagnetic permeability. The observed inverse correlation between field strength and accreted mass can be deduced, by means of the analytic calculation of a proposed crust screen model. The field-period relation P = 2.7 ms B-9(5/7) is also presented, which fits for the equilibrium period line of X-ray binary sources.; Astronomy & Astrophysics; SCI(E); 14; ARTICLE; 3; 889-892; 283
语种	英语
内容类型	期刊论文
源URL	[http://ir.pku.edu.cn/handle/20.500.11897/403206]
专题	地球与空间科学学院
推荐引用方式 GB/T 7714	ZHANG, CM,WU, XJ,YANG, GC. THE CRUST SCREEN MODEL FOR THE MAGNETIC-FIELD OF BINARY-X-RAY SOURCES[J]. astronomy astrophysics,1994.
APA	ZHANG, CM,WU, XJ,&YANG, GC.(1994).THE CRUST SCREEN MODEL FOR THE MAGNETIC-FIELD OF BINARY-X-RAY SOURCES.astronomy astrophysics.
MLA	ZHANG, CM,et al."THE CRUST SCREEN MODEL FOR THE MAGNETIC-FIELD OF BINARY-X-RAY SOURCES".astronomy astrophysics (1994).