ON THE STRUCTURE OF NORMAL SPIRAL GALAXIES WITH FINITE DISK THICKNESS .1. THE MODAL-THEORY

被引：13

作者：

YUE, ZY ^{[1
]}

机构：

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

来源：

关键词：

D O I：

10.1080/03091928208208998

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：1 / 46

页数：46

共 13 条

[1] LOCAL DENSITY-POTENTIAL RELATION FOR SPIRAL DENSITY WAVES IN GALAXIES
BERTIN, G
MARK, JWK
[J]. SIAM JOURNAL ON APPLIED MATHEMATICS, 1979, 36 (03) : 407 - 420
[2] BLAAUW A, 1965, GALACTIC STRUCT, P444
[3] Jeans J. H., 1961, ASTRONOMY COSMOGONY
[4] DISCRETE SPIRAL MODES, SPIRAL WAVES, AND LOCAL DISPERSION RELATIONSHIP
LAU, YY
BERTIN, G
[J]. ASTROPHYSICAL JOURNAL, 1978, 226 (02) : 508 - 520
[5] LIN CC, 1979, STUD APPL MATH, V60, P97
[6] LIN CC, 1970, GALACTIC ASTRONOMY, V2, P1
[7] Nayfeh AH., 1973, PERTURBATION METHODS
[8] NISHIMOTO T, 1979, STUD APPL MATH, V60, P11
[9] ROBERTS WW, 1972, ASTROPHYS LETT COMM, V12, P49
[10] SHU FH, 1968, THESIS HARVARD U