METHOD OF MAPPING COMPACT STRUCTURE IN RADIO-SOURCES USING VLBI OBSERVATIONS

被引：39

作者：

COTTON, WD

机构：

来源：

关键词：

D O I：

10.1086/112519

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：1122 / 1128

页数：7

共 6 条

[1] FORT DN, 1976, ASTRON ASTROPHYS, V50, P19
[2] Hogbom J. A., 1974, Astronomy and Astrophysics Supplement Series, V15, P417
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[4] STRUCTURE OF RADIO-SOURCES 3C 273B AND 3C 84 DEDUCED FROM CLOSURE PHASES AND VISIBILITY AMPLITUDES OBSERVED WITH 3-ELEMENT INTERFEROMETERS
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HINTEREGGER, HF
WHITNEY, AR
COUNSELMAN, CC
SHAPIRO, II
WITTELS, JJ
KLEMPERER, WK
WARNOCK, WW
CLARK, TA
HUTTON, LK
MARANDINO, GE
RONNANG, BO
RYDBECK, OEH
NIELL, AE
[J]. ASTROPHYSICAL JOURNAL, 1974, 193 (02) : 293 - 301
[5] RADIO STRUCTURE OF 3C147 DETERMINED BY MULTI-ELEMENT VERY LONG BASELINE INTERFEROMETRY
WILKINSON, PN
READHEAD, ACS
PURCELL, GH
ANDERSON, B
[J]. NATURE, 1977, 269 (5631) : 764 - 768
[6] TIME-DEPENDENT RADIO FINE-STRUCTURE OF QUASAR 3C-345
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SHAPIRO, II
COTTON, WD
COUNSELMAN, CC
HINTEREGGER, HF
KNIGHT, CA
ROGERS, AEE
WHITNEY, AR
CLARK, TA
HUTTON, LK
NIELL, AE
RONNANG, BO
RYDBECK, OEH
[J]. ASTRONOMICAL JOURNAL, 1976, 81 (11) : 933 - 945