STELLAR DYNAMICS IN THIN DISK GALAXIES .1. UNIFIED APPROACH TO HYDRONAMIC AND ORBIT THEORIES

被引：23

作者：

BERMAN, RH ^{[1
]}

MARK, JWK ^{[1
]}

机构：

[1] MIT,DEPT MATH,CAMBRIDGE,MA 02139

来源：

关键词：

D O I：

10.1086/155468

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：257 / 270

页数：14

共 31 条

[1] BARDEEN JM, 1975, 69 P IAU S DYN STELL
[2] BERMAN RH, 1975, THESIS MIT
[3] Bogoliubov N. N., 1961, ASYMPTOTIC METHODS T
[4] CHANDRASEKHAR S, 1960, PRINCIPLES STELLAR D, P187
[5] Chapman S., 1970, MATH THEORY NONUNIFO, V3rd ed
[6] THE BOLTZMANN EQUATION AND THE ONE-FLUID HYDROMAGNETIC EQUATIONS IN THE ABSENCE OF PARTICLE COLLISIONS
CHEW, GF
GOLDBERGER, ML
LOW, FE
[J]. PROCEEDINGS OF THE ROYAL SOCIETY OF LONDON SERIES A-MATHEMATICAL AND PHYSICAL SCIENCES, 1956, 236 (1204): : 112 - 118
[7] RESONANCE EFFECTS IN SPIRAL GALAXIES
CONTOPOULOS, G
[J]. ASTROPHYSICAL JOURNAL, 1970, 160 (01) : 113 - +
[8] PARTICLE RESONANCE IN SPIRAL GALAXIES - NONLINEAR EFFECTS
CONTOPOULOS, G
[J]. ASTROPHYSICAL JOURNAL, 1973, 181 (03) : 657 - 684
[9] Erickson S.A., 1974, THESIS MIT
[10] FELDMAN SI, 1973, STUD APPL MATH, V52, P1