OPTICAL VARIATIONS IN QUASI-STELLAR OBJECTS

被引：31

作者：

PEACH, JV

机构：

[1] Mount Wilson and Palomar Observatories, Carnegie Institution of Washington

[2] Department of Astrophysics, University Observatory

来源：

NATURE | 1969年 / 222卷 / 5192期

关键词：

D O I：

10.1038/222439a0

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：

Photometric observations of thirty quasi-stellar objects have been made and seven new variables have been discovered. No correlation was found, however, between variability and any other observed property. © 1969 Nature Publishing Group.

引用

页码：439 / &

共 14 条

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[2] 3-COLOR PHOTOMETRY IN THE GLOBULAR CLUSTER M3
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WIRTANEN, CA
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PEACH, JV
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[J]. NATURE, 1969, 221 (5182) : 755 - &
[7] TIME CHANGES IN STRUCTURE OF OPTICAL IMAGE OF 3C 287
MATTHEWS, TA
[J]. ASTROPHYSICAL JOURNAL, 1968, 153 (3P2) : L171 - &
[8] PENSTON MV, IN PRESS
[9] INTENSITY VARIATIONS OF 3C 48 3C 196 + 3C 273 IN OPTICAL WAVELENGTHS
SANDAGE, A
[J]. ASTROPHYSICAL JOURNAL, 1964, 139 (01) : 416 - &
[10] INTENSITY VARIATIONS OF QUASI-STELLAR SOURCES IN OPTICAL WAVELENGTHS
SANDAGE, A
[J]. ASTROPHYSICAL JOURNAL, 1966, 144 (03) : 1234 - &

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