ON THE INTERPRETATION OF THE OBSERVED ANGULAR-SIZE FLUX-DENSITY RELATION FOR EXTRAGALACTIC RADIO-SOURCES

被引：16

作者：

KAPAHI, VK ^{[1
]}

KULKARNI, VK ^{[1
]}

SUBRAHMANYA, CR ^{[1
]}

机构：

[1] TATA INST FUNDAMENTAL RES,CTR RADIO ASTRON,OOTACAMUND 643001,INDIA

来源：

JOURNAL OF ASTROPHYSICS AND ASTRONOMY | 1987年 / 8卷 / 01期

关键词：

D O I：

10.1007/BF02714250

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：33 / 50

页数：18

共 50 条

[31] FLUX-DENSITY MEASUREMENTS OF SELECTED RADIO-SOURCES RELATIVE TO CASSIOPEIA A AT 21.84 GHZ
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[32] MEASUREMENTS OF FLUX-DENSITY OF WEAK RADIO-SOURCES AT FREQUENCIES OF 2.7 AND 10.7 GHZ
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[33] THE LINEAR SIZE EVOLUTION OF EXTRAGALACTIC RADIO-SOURCES REVISITED
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[34] SPECTRAL INDEX - FLUX-DENSITY RELATION FOR EXTRA-GALACTIC RADIO-SOURCES FOUND IN METER-WAVELENGTH SURVEYS
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[35] DETERMINATION OF MEAN ANGULAR SIZE OF SCINTILLATING RADIO-SOURCES AT LOW FLUX DENSITIES
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[36] RELATION OF REDSHIFTS OF RADIO-SOURCES TO THEIR ANGULAR DIAMETERS
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[37] Legacy data and cosmological constraints from the angular-size/redshift relation for ultracompact radio sources
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[39] FLUX-DENSITY MEASUREMENTS OF VARIABLE RADIO-SOURCES AT LAMBDA-8.96 MM (33.5 GHZ)
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[40] The "number-flux density" relation for milliarcsecond structures in extragalactic radio sources
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