A new plasmon solution with centrifugal pressure

被引：6

作者：

Canto, J ^{[1
]}

Espresate, J ^{[1
]}

Raga, AC ^{[1
]}

D'Alessio, P ^{[1
]}

机构：

[1] Natl Autonomous Univ Mexico, Inst Astron, Mexico City 04510, DF, Mexico

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1998年 / 296卷 / 04期

关键词：

hydrodynamics; shock waves; ISM : general;

D O I：

10.1046/j.1365-8711.1998.01472.x

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The 'plasmon' solution of De Young & Axford describes the interaction between a high-velocity clump and the surrounding medium. Even though this solution is probably too simplistic, it has proven to be most useful in the study of diverse astrophysical flows. In the present paper, we discuss a more detailed solution of the plasmon problem, which includes the centrifugal effects of the environmental material flowing around the plasmon. We derive both numerical and approximate analytic solutions of this problem, and compare them with the analytic solution of De Young & Axford.

引用

页码：1041 / 1044

页数：4

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