DO ROTATION CURVES OF SPIRAL GALAXIES IN CLUSTERS DECLINE

被引：27

作者：

AMRAM, P

SULLIVAN, WT

BALKOWSKI, C

MARCELIN, M

CAYATTE, V

机构：

[1] DAEC, OBSERV MEUDON, F-92195 MEUDON, FRANCE

[2] UNIV WASHINGTON, DEPT ASTRON, SEATTLE, WA 98195 USA

来源：

ASTROPHYSICAL JOURNAL | 1993年 / 403卷 / 02期

关键词：

GALAXIES; CLUSTERING; KINEMATICS AND DYNAMICS;

D O I：

10.1086/186721

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Rotation curves for 21 spiral galaxies in five clusters have been obtained in a search for possible effects of the cluster environment on individual galaxy dynamics. We find no significant evidence for anything more than a small influence of the cluster environment. In particular, using 12 selected galaxies we do not confirm the strong correlation between slope of rotation curve and location within a cluster reported by Whitmore, Fobes, & Rubin.

引用

页码：L59 / L62

页数：4

共 18 条

[1]

AMRAM P, 1992, ASTRON ASTROPHYS SUP, V94, P175

[2]

AMRAM P, 1991, THESIS U PROVENCE AI

[3]

AMRAM P, 1991, IN PRESS CLUSTERS GA

[4]

AMRAM P, 1991, IN PRESS DISTRIBUTIO