FLAT ROTATION CURVES - A RESULT OF THE HELICAL INVERSE CASCADE IN TURBULENT MEDIA

被引：3

作者：

PRABHU, RD ^{[1
]}

KRISHAN, V ^{[1
]}

机构：

[1] INDIAN INST SCI,BANGALORE 560012,KARNATAKA,INDIA

来源：

ASTROPHYSICAL JOURNAL | 1994年 / 428卷 / 02期

关键词：

GALAXIES; KINEMATICS AND DYNAMICS; HYDRODYNAMICS; TURBULENCE;

D O I：

10.1086/174261

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We have modeled the rotation curves of 21 galaxies observed by Amram et al. (1992), by combining the effects of rigid rotation, gravity, and turbulence. The main motivation behind such modeling is to study the formation of coherent structures in turbulent media and explore its role in the large-scale structures of the universe. The values of the parameters such as mass, turbulent velocity, and angular velocity derived from the rotation curve fits are in good agreement with those derived from the prevalent models.

引用

页码：483 / 492

页数：10

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