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Physics, Formation and Evolution of Rotating Stars

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Cover of 'Physics, Formation and Evolution of Rotating Stars'

Table of Contents

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    Book Overview
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    Chapter 1 The Mechanical Equilibrium of Stars
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    Chapter 2 The Mechanical Equilibrium of Rotating Stars
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    Chapter 3 The Energetic Equilibrium of Stars
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    Chapter 4 The Energy Conservation and Radiative Equilibrium in Rotating Stars
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    Chapter 5 Stellar Convection
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    Chapter 6 Overshoot, Semiconvection, Thermohaline Convection, Rotation and Solberg–Hoiland Criterion
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    Chapter 7 The Equation of State
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    Chapter 8 The Opacities
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    Chapter 9 Nuclear Reactions and Neutrino Processes
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    Chapter 10 Transport Processes: Diffusion and Advection
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    Chapter 11 Meridional Circulation
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    Chapter 12 Rotation-Driven Instabilities
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    Chapter 13 Magnetic Field Instabilities and Transport Processes
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    Chapter 14 Physics of Mass Loss by Stellar Winds
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    Chapter 15 Radial Pulsations of Stars
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    Chapter 16 Nonradial Stellar Oscillations
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    Chapter 17 Transport by Gravity Waves
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    Chapter 18 Pre-stellar Phase
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    Chapter 19 The Protostellar Phase and Accretion Disks
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    Chapter 20 The Pre-main Sequence Phase and the Birthlines
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    Chapter 21 Rotation in Star Formation
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    Chapter 22 The Formation of Massive Stars
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    Chapter 23 The Formation of First Stars in the Universe: Pop. III and Pop. II.5 Stars
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    Chapter 24 Solutions of the Equations and Simple Models
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    Chapter 25 Evolution in the H-Burning Phases
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    Chapter 26 Evolution in the He Burning and AGB Phases of Low and Intermediate Mass Stars with Rotation
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    Chapter 27 Massive Star Evolution with Mass Loss and Rotation
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    Chapter 28 Advanced Evolutionary Stages and Pre-supernovae
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    Chapter 29 Evolution of Z = 0 and Very Low Z Stars
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About this Attention Score

  • Good Attention Score compared to outputs of the same age (71st percentile)
  • Good Attention Score compared to outputs of the same age and source (67th percentile)

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