THE LONG-TERM EVOLUTION OF ROTATING STELLAR BARS

被引：15

作者：

CARNEVALI, P ^{[1
]}

机构：

[1] IBM CORP,THOMAS J WATSON RES CTR,YORKTOWN HTS,NY 10598

来源：

关键词：

D O I：

10.1086/160714

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：701 / 710

页数：10

共 15 条

[1]

ATHANASSOULA E, 1983, UNPUB

[2]

Binnoy J., 1978, Comments on Astrophysics. Comments on Modern Physics: Part C, V8, P27

[3]

COMBES F, 1981, ASTRON ASTROPHYS, V96, P164

[4] NUMBER OF ISOLATING INTEGRALS IN HAMILTONIAN SYSTEMS [J].

CONTOPOULOS, G ;

GALGANI, L ;

GIORGILLI, A .

PHYSICAL REVIEW A, 1978, 18 (03) :1183-1189

[5]

CONTOPOULOS G, 1974, IAU S, V69, P209

[6]

FROBERG CE, 1965, INTRO NUMERICAL ANAL

[7]

Hohl F., 1969, Journal of Computational Physics, V4, P306, DOI 10.1016/0021-9991(69)90002-3

[8] FREE COLLAPSE OF A ROTATING SPHERE OF STARS [J].

MILLER, RH .

[9] 6 COLLAPSES [J].

MILLER, RH ;

SMITH, BF .

[10] DYNAMICS OF A STELLAR BAR [J].

MILLER, RH ;

SMITH, BF .