THE EVOLUTION OF COMPACT SUPERNOVA-REMNANTS IN A STRONGLY MAGNETIZED MEDIUM

被引：0

作者：

ROZYCZKA, M

TENORIOTAGLE, G

机构：

[1] NICOLAUS COPERNICUS ASTRON CTR,PL-00716 WARSAW,POLAND

[2] INST ASTROFIS CANARIAS,E-38200 LA LAGUNA,SPAIN

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1995年 / 274卷 / 04期

关键词：

ISM; JETS AND OUTFLOWS; ISMM MAGNETIC FIELDS; SUPERNOVA REMNANTS; GALAXIES; ACTIVE;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Two-dimensional simulations of the evolution of supernova remnants in a uniform, high-density medium are presented. The medium is magnetized, and its magnetic pressure is much larger than the thermal pressure. The evolution of the remnants is followed past full thermalization of the ejecta. A mechanism of self-collimation of the flow is identified, resulting in formation of jets that propagate along the magnetic field lines.

引用

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页码：1157 / 1164

页数：8

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