SPECTRAL PROPERTIES OF X-RAY OBJECTS GX 3+1 GX 354-5 AND SCO XR-1

被引：30

作者：

BUSELLI, G

CLANCY, MC

DAVISON, PJN

EDWARDS, PJ

MCCRACKE.KG

THOMAS, RM

机构：

[1] Department of Physics, University of Otago, Dunedin

来源：

NATURE | 1968年 / 219卷 / 5159期

关键词：

D O I：

10.1038/2191124a0

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：

The spectra of three X-ray objects have been measured from a balloon, and suggest that the sources are supernova remnants, and that the X-ray emission is due to magnetic bremsstrahlung. © 1968 Nature Publishing Group.

引用

页码：1124 / &

共 7 条

[1] EXTENDED SOURCE OF ENERGETIC COSMIC X RAYS
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MCDONALD, FB
RIEGLER, G
SERLEMITSOS, P
[J]. PHYSICAL REVIEW LETTERS, 1966, 17 (08) : 447 - +
[2] BRADT H, IN PRESS
[3] DISTRIBUTION AND VARIABILITY OF COSMIC X-RAY SOURCES
FRIEDMAN, H
BYRAM, ET
CHUBB, TA
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[4] DISTRIBUTION OF GALACTIC X-RAY SOURCES FROM SCORPIO TO CYGNUS
GURSKY, H
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GIACCONI, R
[J]. ASTROPHYSICAL JOURNAL, 1967, 150 (2P2) : L75 - &
[5] BALLOON X-RAY ASTRONOMY
PETERSON, LE
JERDE, RL
JACOBSON, AS
[J]. AIAA JOURNAL, 1967, 5 (11) : 1921 - +
[6] SPECTRUM OF SCORPIUS XR-1 TO 50 KEV
PETERSON, LE
JACOBSON, AS
[J]. ASTROPHYSICAL JOURNAL, 1966, 145 (03) : 962 - &
[7] PETERSON LE, 1968, 10 P INT C COSM RAYS

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