THE DISTANCE TO TYCHOS SUPER-NOVA REMNANT (3C10) - A REDISCUSSION

被引：20

作者：

SCHWARZ, UJ

ARNAL, EM

GOSS, WM

机构：

[1] Kapteyn Astronomical Institute, University of Groningen, Groningen, Netherlands

[2] Instituto Argentino de Radioastronomia and Observatorio Astronomico La Plata, Argentina

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1980年 / 192卷 / 03期

关键词：

D O I：

10.1093/mnras/192.1.67P

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：P67 / P71

页数：5

共 12 条

[1]

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[3]

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[4]

GOSS WM, 1973, ASTR ASTROPHYS, V28, P309

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[6] STRUCTURE OF TYCHO SUPER-NOVA REMNANT [J].

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[7] EXPANSION OF OPTICAL REMNANT OF TYCHOS SUPER-NOVA [J].

KAMPER, KW ;

VANDENBERGH, S .

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[8] RADIAL VELOCITIES AND KINEMATICS OF GALACTIC H PI REGIONS [J].

MILLER, JS .

ASTROPHYSICAL JOURNAL, 1968, 151 (2P1) :473-&

[9] OPTICAL AND RADIO EVIDENCE OF LARGE-SCALE PECULIAR MOTIONS IN CASSIOPEIA-PERSEUS ARM [J].

RICKARD, JJ .

ASTROPHYSICAL JOURNAL, 1968, 152 (3P1) :1019-&

[10]

ROHLFS K, 1974, ASTRON ASTROPHYS, V35, P177

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