On the orbit structure of the logarithmic potential

被引:30
作者
Belmonte, C.
Boccaletti, D.
Pucacco, G.
机构
[1] Univ Roma La Sapienza, Dept Phys, I-00185 Rome, Italy
[2] Univ Roma La Sapienza, Dept Math, I-00185 Rome, Italy
[3] Univ Roma Tor Vergata, Dept Phys, I-00133 Rome, Italy
[4] Ist Nazl Fis Nucl, Sez Roma Tor Vergata, Rome, Italy
关键词
galaxies : kinematics and dynamics; methods : analytical;
D O I
10.1086/521423
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We investigate the dynamics in the logarithmic galactic potential with an analytical approach. The phase-space structure of the real system is approximated with resonant detuned normal forms constructed with the method based on the Lie transform. Attention is focused on the properties of the axial periodic orbits and of low-order ``boxlets'' that play an important role in galactic models. Using energy and ellipticity as parameters, we find analytical expressions of several useful indicators, such as stability-instability thresholds, bifurcations, and phase- space fractions of some orbit families, and compare them with numerical results available in the literature.
引用
收藏
页码:202 / 217
页数:16
相关论文
共 43 条