HYDRODYNAMIC INSTABILITIES AND FORMATION OF RADIO SHELLS IN YOUNG SUPERNOVAE REMNANTS

被引:16
作者
COWIE, LL [1 ]
机构
[1] HARVARD UNIV,PHYS DEPT,CAMBRIDGE,MA 02138
关键词
D O I
10.1093/mnras/173.2.429
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:429 / 436
页数:8
相关论文
共 22 条
[1]   STRUCTURE AND EVOLUTION OF PLANETARY-NEBULAE [J].
CAPRIOTTI, ER .
ASTROPHYSICAL JOURNAL, 1973, 179 (02) :495-516
[2]  
Chandrasekhar S., 1961, HYDRODYNAMIC HYDROMA
[3]   ON ELEPHANT-TRUNK STRUCTURES IN THE REGION OF O-ASSOCIATIONS [J].
FRIEMAN, EA .
ASTROPHYSICAL JOURNAL, 1954, 120 (01) :18-21
[4]   INTERPRETATION OF RADIO EMISSION FROM SUPERNOVA REMNANTS CASA AND 3C10 [J].
GULL, SF .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1973, 162 (02) :135-142
[5]   NUMERICAL MODEL OF STRUCTURE AND EVOLUTION OF YOUNG SUPERNOVA REMNANTS [J].
GULL, SF .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1973, 161 (01) :47-69
[6]   POLARIMETRIC APERTURE SYNTHESIS OBSERVATIONS OF 4 SMALL-DIAMETER SUPERNOVA REMNANTS [J].
HERMANN, BR ;
DICKEL, JR .
ASTRONOMICAL JOURNAL, 1973, 78 (09) :879-&
[7]  
KAHN FS, 1973, P NATO C
[8]  
KAHN FS, 1974, LECTURE LES HOUCHES
[9]  
KULSRUD RM, 1965, ASTROPHYS J, V142, P491, DOI 10.1086/148314
[10]  
MCKEE CF, TO BE PUBLISHED