標(biāo)題: Titlebook: Stability of Collisionless Stellar Systems; Mechanisms for the D P. L. Palmer Book 1994 Springer Science+Business Media Dordrecht 1994 Cosm [打印本頁] 作者: 適婚女孩 時(shí)間: 2025-3-21 17:55
書目名稱Stability of Collisionless Stellar Systems影響因子(影響力)
書目名稱Stability of Collisionless Stellar Systems影響因子(影響力)學(xué)科排名
書目名稱Stability of Collisionless Stellar Systems網(wǎng)絡(luò)公開度
書目名稱Stability of Collisionless Stellar Systems網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Stability of Collisionless Stellar Systems被引頻次
書目名稱Stability of Collisionless Stellar Systems被引頻次學(xué)科排名
書目名稱Stability of Collisionless Stellar Systems年度引用
書目名稱Stability of Collisionless Stellar Systems年度引用學(xué)科排名
書目名稱Stability of Collisionless Stellar Systems讀者反饋
書目名稱Stability of Collisionless Stellar Systems讀者反饋學(xué)科排名
作者: 原告 時(shí)間: 2025-3-21 21:09
https://doi.org/10.1007/978-94-017-3059-4Cosmology; Galaxy; astronomy; simulation; stellar作者: reaching 時(shí)間: 2025-3-22 00:50 作者: Pastry 時(shí)間: 2025-3-22 05:14 作者: Conclave 時(shí)間: 2025-3-22 11:42 作者: 美色花錢 時(shí)間: 2025-3-22 13:56 作者: 死亡率 時(shí)間: 2025-3-22 18:46
General Perturbation Theory,ual stars and thus we cannot infer anything about collective instability in the system, which requires a self-consistent build up of the combination of the perturbations to all the orbits of the stars in the system. A good account of the use of action and angle variables in perturbation theory can be found in [30].作者: Cubicle 時(shí)間: 2025-3-22 22:40 作者: SPASM 時(shí)間: 2025-3-23 02:06 作者: 滲入 時(shí)間: 2025-3-23 07:01
Description of the Orbital Motions,dels with at least one axis of symmetry. The results derived in this chapter will provide the groundwork for the next chapter where we shall consider the effects of perturbing the equilibrium potential that governs the motions of the stars.作者: Hallowed 時(shí)間: 2025-3-23 10:16 作者: 證明無罪 時(shí)間: 2025-3-23 16:23 作者: 油膏 時(shí)間: 2025-3-23 21:34 作者: enhance 時(shí)間: 2025-3-23 23:46
Axisymmetric Systems, the matrix equation for general integrable systems, and apply it to axisymmetric systems. The apparatus, however, is ready for extension to triaxial St?ckel systems. We shall keep our discussion independent of any specific models, although models of self-consistent axisymmetric St?ckel systems have been built [50, 29].作者: hair-bulb 時(shí)間: 2025-3-24 05:28 作者: Lipoma 時(shí)間: 2025-3-24 10:29
Introduction,galaxies may have been formed from just looking at their dynamics today. In this introduction I hope to set out why I believe that studying unstable models of galaxies can lead to an understanding of the answers to these two fundamental questions.作者: Restenosis 時(shí)間: 2025-3-24 13:31 作者: Foregery 時(shí)間: 2025-3-24 16:43 作者: 文藝 時(shí)間: 2025-3-24 22:22 作者: Bernstein-test 時(shí)間: 2025-3-25 01:31 作者: Fsh238 時(shí)間: 2025-3-25 06:36 作者: Biguanides 時(shí)間: 2025-3-25 09:43
Description of the Orbital Motions,at the motion of individual stars within the galaxies, show how their motions are determined, and introduce different notations that will prove useful in the description of these motions. We will consider three kinds of systems in this book, spherical systems, axisymmetric systems and disc systems. 作者: 休閑 時(shí)間: 2025-3-25 11:45
General Perturbation Theory,e the theory for a number of cases which will be of interest to us later. It is important to note that in this section we are only considering individual stars and thus we cannot infer anything about collective instability in the system, which requires a self-consistent build up of the combination o作者: Observe 時(shí)間: 2025-3-25 18:00
Constructing Equilibrium Models,f because although there are a lot of models in the literature, our aim in this book is to discuss stability in general terms, rather than stability of individual models. Discussion of various equilibrium models can be found in [45] and [56]. We shall set out the general principles of model building作者: Anonymous 時(shí)間: 2025-3-25 21:44 作者: 雪崩 時(shí)間: 2025-3-26 03:11
Isotropic Systems,r, discuss what we may learn from this matrix equation for stellar systems in which the pressure from random motions is isotropic. Such systems were, for a long time, thought to be the most appropriate to describe elliptical galaxies with the further restriction that their distribution function decr作者: 賄賂 時(shí)間: 2025-3-26 04:50 作者: chalice 時(shí)間: 2025-3-26 10:18 作者: Malleable 時(shí)間: 2025-3-26 16:21 作者: Evacuate 時(shí)間: 2025-3-26 17:47 作者: 停止償付 時(shí)間: 2025-3-26 23:59
Non-Linear Evolution and Endstates,numerical tools for following the evolution of these instabilities from the linear through the non-linear regime to a final stable end configuration. In this chapter we shall discuss the results obtained with the smooth potential technique used to follow the non-linear evolution of the instabilities作者: PATRI 時(shí)間: 2025-3-27 01:31
Disc Galaxies,though these systems are notoriously unstable. One of the problems with discussing disc galaxies is that they contain a large amount of gas and, due to the spiral structure, a lot of active star formation. Our analysis has assumed a given distribution function which is time independent and does not 作者: 擁擠前 時(shí)間: 2025-3-27 06:17
Norased Nasongklay study the highly specialized genetic literature available. This book is an attempt to fill this void. We have made an effort to keep it as short and clear as possible and to limit it to the important and most frequent genetic abnor- malities. In particular, we have tried to take into consid- erati作者: 孵卵器 時(shí)間: 2025-3-27 12:48 作者: palette 時(shí)間: 2025-3-27 13:55 作者: 熱情贊揚(yáng) 時(shí)間: 2025-3-27 20:43 作者: Autobiography 時(shí)間: 2025-3-27 22:15 作者: doxazosin 時(shí)間: 2025-3-28 06:07 作者: Narcissist 時(shí)間: 2025-3-28 08:04 作者: Anhydrous 時(shí)間: 2025-3-28 14:04 作者: 影響 時(shí)間: 2025-3-28 15:36 作者: 粗魯性質(zhì) 時(shí)間: 2025-3-28 19:10
V. V. Apollonovips between different sign systems, be they verbal or nonverbal. The chapter will conclude with an overview on the musical phenomena discussed within the scope of Translation Studies and indicate the potential area of overlap between translation studies and musicology.作者: motivate 時(shí)間: 2025-3-29 00:09 作者: 鞏固 時(shí)間: 2025-3-29 05:58 作者: 昏迷狀態(tài) 時(shí)間: 2025-3-29 09:48 作者: Dawdle 時(shí)間: 2025-3-29 14:00 作者: defenses 時(shí)間: 2025-3-29 16:41
Front Matterdungen bilden sollen, die als selbst?ndige Phasen am Gleichgewicht teilnehmen, sondern nur physikalische Gemenge oder L?sungen (vgl. .: Lehrbuch, 11. Aufl., S. 105). Eine allgemeine Definition des Begriffes der L?sungen ist bereits früher (S. 129) gegeben worden. Solche L?sungen k?nnen in allen drei作者: 庇護(hù) 時(shí)間: 2025-3-29 22:21
ntainers, including tips and shortcuts to make everyday tasks easier. Databases have unique demands for performance and reliability, and this book addresses those qualities with discussions on protecting, persi978-1-4842-9032-3978-1-4842-9033-0
