FROM ROTATIONS AND INCLINATIONS TO ZERO CONFIGURATIONAL VELOCITY SURFACES .2. THE BEST POSSIBLE CONFIGURATIONAL VELOCITY SURFACES

被引：15

作者：

SAARI, DG

机构：

来源：

CELESTIAL MECHANICS | 1987年 / 40卷 / 3-4期

关键词：

D O I：

10.1007/BF01235841

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：197 / 223

页数：27

共 18 条

[1] ZERO VELOCITY SURFACES FOR GENERAL PLANAR 3-BODY PROBLEM [J].

BOZIS, G .

[2] SOME TOPOLOGY OF 3-BODY PROBLEMS [J].

EASTON, R .

[3]

GOLUBEV V, 1968, SOVIET PHYSICS DOKLA, P373

[4]

GOLUBEV V, 1967, SOVIET PHYSICS DOKLA, P527

LASKAR, J .

CELESTIAL MECHANICS, 1984, 32 (01) :15-28

[6] FINAL EVOLUTION OF N-BODY PROBLEM [J].

MARCHAL, C ;

SAARI, DG .

[7] HILL REGIONS FOR GENERAL 3-BODY PROBLEM [J].

MARCHAL, C ;

SAARI, DG .

CELESTIAL MECHANICS, 1975, 12 (02) :115-129

[8] RELATIVE EQUILIBRIA AND THE VIRIAL THEOREM [J].

PALMORE, JI .

CELESTIAL MECHANICS, 1979, 19 (02) :167-171

[9]

Saari D. G., 1970, Periodic orbits, stability and resonances, P76

[10]

Saari D. G., 1983, Motion of Planets and Natural and Artificial Satellites. Proceedings of a CNPq-NSF Symposium and Workshop, P27