EXTENDED ROTATION CURVES OF HIGH-LUMINOSITY SPIRAL GALAXIES .5. NGC-1961, THE MOST MASSIVE SPIRAL KNOWN

被引：37

作者：

RUBIN, VC ^{[1
]}

FORD, WK ^{[1
]}

ROBERTS, MS ^{[1
]}

机构：

[1] NATL RADIO ASTRON OBSERV,GREEN BANK,WV 24944

来源：

ASTROPHYSICAL JOURNAL | 1979年 / 230卷 / 01期

关键词：

D O I：

10.1086/157059

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：35 / 39

页数：5

共 12 条

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[5]

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[6]

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[8]

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[9] EXTENDED ROTATION CURVES OF HIGH-LUMINOSITY SPIRAL GALAXIES .4. SYSTEMATIC DYNAMICAL PROPERTIES SA-]SC [J].

RUBIN, VC ;

FORD, WK ;

THONNARD, N .

ASTROPHYSICAL JOURNAL, 1978, 225 (03) :L107-L111

[10] STEPS TOWARD HUBBLE CONSTANT .7. DISTANCES TO NGC 2403, M101, AND VIRGO CLUSTER USING 2U CENTIMETER LINE WIDTHS COMPARED WITH OPTICAL METHODS - GLOBAL VALUE OF HO [J].

SANDAGE, A ;

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ASTROPHYSICAL JOURNAL, 1976, 210 (01) :7-&

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