HIGH-ENERGY X-RAY OBSERVATIONS OF A LUNAR OCCULTATION OF CRAB-NEBULA

被引：24

作者：

RICKER, GR

SCHEEPMAKER, A

RYCKMAN, SG

BALLINTINE, JE

DOTY, JP

DOWNEY, PM

LEWIN, WHG

机构：

[1] MIT,PHYS DEPT,BLDG 37,CAMBRIDGE,MA 02139

[2] MIT,CTR SPACE RES,CAMBRIDGE,MA

来源：

ASTROPHYSICAL JOURNAL | 1975年 / 197卷 / 02期

关键词：

D O I：

10.1086/181784

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：L83 / &

共 22 条

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[12]

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[13]

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[16] ACTIVITY IN CRAB NEBULA FOLLOWING PULSAR SPIN-UP OF 1969 SEPTEMBER [J].

SCARGLE, JD ;

HARLAN, EA .

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[17]

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[18]

STAUBERT R, 1975, PRIVATE COMMUNICATIO

[19] DISTANCE TO CRAB-NEBULA AND NP-0532 [J].

TRIMBLE, V .

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 1973, 85 (507) :579-585

[20] STRUCTURE OF CRAB-NEBULA AT 2.7 AND 5 GHZ .1. OBSERVATIONS [J].

WILSON, AS .

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