Titlebook: Stellar Pulsation - Nonlinear Studies; Mine Takeuti,Dimitar D. Sasselov Book 2001 Springer Science+Business Media B.V. 2001 simulation.sta

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A Historical Sketch of the Beat Cepheid Studies,e secondary bumps defining the Hertzsprung progression in Cepheid light curves and of Cepheids in open clusters with known distances gave two types of pulsation masses about 40% smaller than the estimated evolution masses. In contrast, the estimated beat masses were a factor of 2–3 smaller than the

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The Multiperiodic Behavior of RR Lyrae Stars,riodic variables among RR Lyrae stars. Especially interesting are those with long-period amplitude and phase modulations. Due to the central role of RR Lyrae stars in many astrophysical issues (distance scale, Pop. II stellar evolution, Galactic structure, etc.), understanding these variables has a

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RV Tauri Stars,rnating pulsations of these variables, and discuss their relation to the period doubling phenomenon in W Virginis stars. We also discuss the period-luminosity relation for RV Tauri stars, recently obtained following the MACHO survey of the LMC stars, and compare it to the theoretical prediction. The

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The Model-Oscillators of Stellar Pulsation,ons with nonlinear terms which cause irregular and chaotic oscillations. The Lorenz equation and its family are described. One of them, the Moore and Spiegel equation is mentioned as one of the simplest dissipative chaotic jerk equations. One-zone models not only for pulsation but also for convectio

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Titlebook: Stellar Pulsation - Nonlinear Studies; Mine Takeuti,Dimitar D. Sasselov Book 2001 Springer Science+Business Media B.V. 2001 simulation.sta

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