MAGNETOHYDRODYNAMIC MODEL OF CRAB-NEBULA RADIATION

被引：516

作者：

KENNEL, CF

CORONITI, FV

机构：

[1] UNIV CALIF LOS ANGELES,CTR PLASMA PHYS & FUS ENGN,LOS ANGELES,CA 90024

[2] UNIV CALIF LOS ANGELES,DEPT PHYS & ASTRON,LOS ANGELES,CA 90024

来源：

ASTROPHYSICAL JOURNAL | 1984年 / 283卷 / 02期

关键词：

D O I：

10.1086/162357

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：710 / 730

页数：21

共 55 条

[1]

[Anonymous], 1975, RAD PROCESSES ASTROP

[2]

ARONS J, 1979, SPACE SCI REV, V24, P437, DOI 10.1007/BF00172212

[3]

ARONS J, 1983, COMMUNICATION

[4]

ASCHENBACH B, 1975, ASTRON ASTROPHYS, V41, P147

[5]

Axford W. I., 1977, P 15 INT C COSM RAYS, V11, P132

[6] PARTICLE ACCELERATION BY ASTROPHYSICAL SHOCKS [J].

BLANDFORD, RD ;

OSTRIKER, JP .

ASTROPHYSICAL JOURNAL, 1978, 221 (01) :L29-L32

[7]

CHENG A, 1982, COMMUNICATION

[8] X-RAY-EMISSION FROM RADIO PULSAR WINDS [J].

CHENG, AF .

ASTROPHYSICAL JOURNAL, 1983, 275 (02) :790-801

[9]

CHEVALIER RA, 1977, SUPERNOVAE, P53

[10] 3-DIMENSIONAL STRUCTURE OF THE CRAB-NEBULA [J].

CLARK, DH ;

MURDIN, P ;

WOOD, R ;

GILMOZZI, R ;

DANZIGER, J ;

FURR, AW .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1983, 204 (01) :415-&

← 1 2 3 4 5 6 →