SELF-CONSISTENT MODELS OF SPIRAL GALAXIES

被引:0
|
作者
CONTOPOULOS, G [1 ]
机构
[1] UNIV ATHENS, DEPT ASTRON, ATHENS, GREECE
关键词
D O I
暂无
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
引用
收藏
页码:101 / 113
页数:13
相关论文
共 50 条
  • [21] SELF-CONSISTENT EVOLUTION OF RING GALAXIES
    MAZZEI, P
    CURIR, A
    BONOLI, C
    ASTRONOMICAL JOURNAL, 1995, 110 (02): : 559 - 572
  • [22] RING GALAXIES WITH SELF-CONSISTENT HALOES
    HUANG, SN
    STEWART, P
    ASTRONOMY & ASTROPHYSICS, 1988, 197 (1-2) : 14 - 28
  • [23] ELLIPTIC GALAXIES WITH DARK MATTER .1. SELF-CONSISTENT MODELS
    BERTIN, G
    SAGLIA, RP
    ASTROPHYSICAL JOURNAL, 1992, 384 (02): : 423 - 432
  • [24] Kolmogorov-Sinai entropy in self-consistent models of barred galaxies
    Wozniak, H
    Pfenniger, D
    XVTH IAP MEETING DYNAMICS OF GALAXIES: FROM THE EARLY UNIVERSE TO THE PRESENT, 2000, 197 : 77 - 78
  • [25] Self-consistent models of cuspy triaxial galaxies with dark matter halos
    Capuzzo-Dolcetta, R.
    Leccese, L.
    Merritt, D.
    Vicari, A.
    ASTROPHYSICAL JOURNAL, 2007, 666 (01): : 165 - 180
  • [26] Nearly self-consistent disc-bulge-halo models for galaxies
    Kuijken, K
    Dubinski, J
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1995, 277 (04) : 1341 - 1353
  • [27] Self-consistent models of triaxial cuspy galaxies with dark matter halos
    Capuzzo-Dolcetta, R.
    Leccese, L.
    Merritt, D.
    Vicari, A.
    PATHWAYS THROUGH AN ECLECTIC UNIVERSE, 2008, 390 : 491 - +
  • [28] SELF-CONSISTENT STATIONARY MODELS OF 2D BARRED GALAXIES
    DEBBASCH, F
    NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA B-GENERAL PHYSICS RELATIVITY ASTRONOMY AND MATHEMATICAL PHYSICS AND METHODS, 1992, 107 (10): : 1099 - 1106
  • [29] Foundations of self-consistent particle-rotor models and of self-consistent cranking models
    Klein, A
    PHYSICAL REVIEW C, 2001, 63 (01): : 143161 - 1431616
  • [30] A self-consistent model of the spiral structure of the galaxy
    Amaral, LH
    Lepine, JRD
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1997, 286 (04) : 885 - 894