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Titlebook: Observational Manifestation of Chaos in Astrophysical Objects; Invited talks for a Alexei M. Fridman,Mikhail Ya. Marov,Richard H. Mil Book

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樓主: CHARY
11#
發(fā)表于 2025-3-23 12:16:53 | 只看該作者
12#
發(fā)表于 2025-3-23 17:41:35 | 只看該作者
13#
發(fā)表于 2025-3-23 19:50:34 | 只看該作者
14#
發(fā)表于 2025-3-23 23:04:15 | 只看該作者
http://image.papertrans.cn/o/image/700364.jpg
15#
發(fā)表于 2025-3-24 03:01:32 | 只看該作者
16#
發(fā)表于 2025-3-24 07:18:15 | 只看該作者
17#
發(fā)表于 2025-3-24 10:46:16 | 只看該作者
Observational Manifestations of Precession of Accretion Disk in the SS 433 Binary System,Basic properties of the unique object SS 433 are described. Observational spectroscopic and photometric manifestations of a precessing accretion disk around a relativistic object in this X-ray binary system are presented.
18#
發(fā)表于 2025-3-24 14:58:02 | 只看該作者
Should Elliptical Galaxies be Idealised as Collisionless Equilibria?,This review summarises several different lines of argument suggesting that one should not expect cuspy nonaxisymmetric galaxies to exist as robust, long-lived collisionless equilibria, ., that such objects should not be idealised as time-independent solutions to the collisionless Boltzmann equation.
19#
發(fā)表于 2025-3-24 21:58:27 | 只看該作者
Orbits and Integrals in Self-Consistent Systems,the (1979) computer program. The nonresonant form of the third integral explains the box orbits, while a resonant form of this integral explains both the box orbits and the 1:1 tube orbits. The N-body model gives the distribution of velocities ., which is an exponential of the third integral.
20#
發(fā)表于 2025-3-25 03:09:01 | 只看該作者
Resonantly Excited Non-Linear Density Waves in Disk Systems,n a highly non-linear responses in the disk. Therefore, non-linear theory is a necessity here. We will examine the non-linear theory of resonance excitation and discuss the applications of the theory to Saturn’s rings and disk galaxies in this paper.
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