RADIATION FROM A STRONGLY-MAGNETIZED PLASMA - THE CASE OF PREDOMINANT SCATTERING

被引：69

作者：

KAMINKER, AD

PAVLOV, GG

SHIBANOV, YA

机构：

来源：

关键词：

D O I：

10.1007/BF00683336

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：249 / 297

页数：49

共 40 条

[1] PHOTON SPLITTING AND PHOTON DISPERSION IN A STRONG MAGNETIC FIELD
ADLER, SL
[J]. ANNALS OF PHYSICS, 1971, 67 (02) : 599 - &
[2] Basko M. M., 1976, ASTROPHYSICS, V12, P169
[3] LIMITING LUMINOSITY OF ACCRETING NEUTRON STARS WITH MAGNETIC-FIELDS
BASKO, MM
SUNYAEV, RA
[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1976, 175 (02) : 395 - 417
[4] BASKO MM, 1975, ASTRON ASTROPHYS, V42, P311
[5] CLASSICAL CALCULATION OF THOMSON CROSS-SECTIONS IN THE PRESENCE OF A STRONG MAGNETIC-FIELD
BORNER, G
MESZAROS, P
[J]. PLASMA PHYSICS AND CONTROLLED FUSION, 1979, 21 (04) : 357 - 367
[6] THOMSON SCATTERING IN A STRONG MAGNETIC FIELD
CANUTO, V
LODENQUA.J
RUDERMAN, M
[J]. PHYSICAL REVIEW D, 1971, 3 (10): : 2303 - &
[7] Dolginov A. Z., 1979, PROPAGATION POLARIZA
[8] FELTEN JE, 1972, ASTRON ASTROPHYS, V17, P226
[9] GNEDIN YN, 1978, JETP LETT+, V27, P305
[10] GNEDIN YN, 1974, ASTRON ASTROPHYS, V36, P379