QUASISTELLAR OBJECTS AND SEYFERT GALAXIES

被引：5

作者：

COLGATE, SA

机构：

来源：

PHYSICS TODAY | 1969年 / 22卷 / 01期

关键词：

D O I：

10.1063/1.3035354

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

Are these two classes of distant objects related Evolution of dense stellar clusters, so crowded with stars that collisions occur, yielding more massive stars and supernovae, could be the common origin of them both. © 1969, American Institute of Physics. All rights reserved.

引用

页码：27 / &

共 19 条

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BURBIDGE, GR
FOWLER, WA
HOYLE, F
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[3] BURBIDGE EM, 1963, REV MOD PHYS, V35, P947
[4] ENHANCEMENT OF LIGHT OUTPUT FROM A SUPERNOVA
COLGATE, SA
CAMERON, AGW
[J]. NATURE, 1963, 200 (490) : 870 - &
[5] STELLAR COALESCENCE AND MULTIPLE SUPERNOVA INTERPRETATION OF QUASI-STELLAR SOURCES
COLGATE, SA
[J]. ASTROPHYSICAL JOURNAL, 1967, 150 (1P1) : 163 - +
[6] COLGATE SA, 1968, APR AM ASTR SOC M CH
[7] DEYOUNG PS, 1967, NUOVO CIMENTO, P199
[8] MICROWAVE SCATTERING FROM UNSTABLE PLASMA WAVES
DRUMMOND, WE
[J]. PHYSICS OF FLUIDS, 1962, 5 (09) : 1133 - 1134
[9] GOLD T, 1965, QUASISTELLAR SOURCES, P93
[10] MINKOWSKI R, 1967, STARS STELLAR SYSTEM, V7, pCH11

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