SOME MODELS FOR EMISSION-LINE REGION OF 3C 48

被引：39

作者：

BAHCALL, JN

KOZLOVSK.BZ

机构：

来源：

关键词：

D O I：

10.1086/150216

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：529 / &

共 12 条

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[2] SENSITIVITY OF SOLAR-NEUTRINO FLUXES
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[3] ON INTERPRETATION OF LINE SPECTRA OF QUASI-STELLAR OBJECTS
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[4] QUASI-STELLAR RADIO SOURCES 3C 48 + 3C 273
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SCHMIDT, M
[J]. ASTROPHYSICAL JOURNAL, 1964, 140 (01) : 1 - &
[5] RED-SHIFT OF UNUSUAL RADIO SOURCE - 3C 48
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MATTHEWS, TA
[J]. NATURE, 1963, 197 (487) : 1041 - &
[6] House L. L., 1964, ASTROPHYS J SUPPL S, V8, P307, DOI 10.1086/190091
[7] OKE B, 1969, PRIVATE COMMUNICATIO
[8] OKE B, 1966, ASTROPHYS J, V145, P668
[9] EXCITATION OF OPTICAL EMISSION LINES IN QUASI-STELLAR RADIO SOURCES
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[J]. ASTROPHYSICAL JOURNAL, 1966, 143 (01) : 268 - +
[10] SHKLOVSK.IS, 1965, SOV ASTRON, V8, P638