FINE-STRUCTURE IN THE NORTHERN EXTENSION OF THE MAGELLANIC STREAM

被引：6

作者：

ERKES, JW

PHILIP, AGD

TURNER, KC

机构：

[1] UNION UNIV UNION COLL,SCHENECTADY,NY 12308

[2] CARNEGIE INST WASHINGTON,DEPT TERR MAGNETISM,WASHINGTON,DC 20005

来源：

ASTROPHYSICAL JOURNAL | 1980年 / 238卷 / 02期

关键词：

D O I：

10.1086/158010

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：546 / 553

页数：8

共 10 条

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[4] SIMULATION OF MAGELLANIC STREAM TO ESTIMATE TOTAL MASS OF MILKY-WAY [J].

LIN, DNC ;

LYNDENBELL, D .

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[5] MAGELLANIC STREAM - TURBULENT WAKE OF MAGELLANIC CLOUDS IN HALO OF GALAXY [J].

MATHEWSON, DS ;

SCHWARZ, MP ;

MURRAY, JD .

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[9] UNUSUAL HIGH-VELOCITY HYDROGEN FEATURE [J].

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WRIXON, GT .

ASTROPHYSICAL JOURNAL, 1972, 173 (03) :L119-&

[10]

Williams D. R. W., 1973, Astronomy and Astrophysics Supplement Series, V8, P505

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