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1.

図書

図書
edited by Alessandro Sozzetti, Mario G. Lattanzi and Alan P. Boss
出版情報: Cambridge : Cambridge University Press, 2011  xxx, 563 p. ; 26 cm
シリーズ名: IAU Symposium and Colloquium proceedings series ; 276
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Planet Formation / Part I:
Structure and Atmospheres / Part II:
Interactions / Part III:
The Next Decade / Part IV:
Poster Papers / Part V:
Planet Formation / Part I:
Structure and Atmospheres / Part II:
Interactions / Part III:
2.

図書

図書
Philip J. Armitage
出版情報: New York : Cambridge University Press, 2010  x, 284 p. ; 26 cm
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Preface
Observations of planetary systems / 1:
Solar System planets / 1.1:
The minimum mass Solar Nebula / 1.1.1:
Minor bodies in the Solar System / 1.2:
Radioactive dating of the Solar System / 1.3:
The snowline in the Solar Nebula / 1.4:
Chondritic meteorites / 1.5:
Extrasolar planetary systems / 1.6:
Direct imaging / 1.6.1:
Radial velocity searches / 1.6.2:
Astrometry / 1.6.3:
Transits / 1.6.4:
Gravitational microlensing / 1.6.5:
Properties of extrasolar planets / 1.7:
Further reading / 1.8:
Protoplanetary disk structure / 2:
Disks in the context of star formation / 2.1:
Classification of Young Stellar Objects / 2.1.1:
Vertical structure / 2.2:
Radial force balance / 2.3:
Radial temperature profile of passive disks / 2.4:
Razor-thin disks / 2.4.1:
Flared disks / 2.4.2:
Radiative equilibrium disks / 2.4.3:
The Chiang-Goldreich model / 2.4.4:
Spectral energy distributions / 2.4.5:
Opacity / 2.5:
Opacity in the optically thin outer disk / 2.5.1:
Analytic opacities / 2.5.2:
The condensation sequence / 2.6:
Ionization state of protoplanetary disks / 2.7:
Thermal ionization / 2.7.1:
Nonthermal ionization / 2.7.2:
Protoplanetary disk evolution / 2.8:
Observations of disk evolution / 3.1:
Surface density evolution of a thin disk / 3.2:
The viscous time scale / 3.2.1:
Solutions to the disk evolution equation / 3.2.2:
Temperature profile of accreting disks / 3.2.3:
Vertical structure of protoplanetary disks / 3.3:
The central temperature of accreting disks / 3.3.1:
Shakura-Sunyaev ? prescription / 3.3.2:
Vertically averaged solutions / 3.3.3:
Angular momentum transport mechanisms / 3.4:
The Rayleigh criterion / 3.4.1:
The magnetorotational instability / 3.4.2:
Disk winds and magnetic braking / 3.4.3:
Hydrodynamic turbulence / 3.4.4:
Fffects of partial ionization on disk evolution / 3.5:
Layered disks / 3.5.1:
Disk dispersal / 3.6:
Photoevaporation / 3.6.1:
Viscous evolution with photoevaporation / 3.6.2:
Magnetospheric accretion / 3.7:
Planetesiroal formation / 3.8:
Aerodynamic drag on solid particles / 4.1:
Epstein drag / 4.1.1:
Stokes drag / 4.1.2:
Dust settling / 4.2:
Single particle settling with coagulation / 4.2.1:
Settling in the presence of turbulence / 4.2.2:
Radial drift of solid particles / 4.3:
Radial drift with coagulation / 4.3.1:
Particle concentration at pressure maxima / 4.3.2:
Turbulent radial diffusion / 4.3.3:
Diffusion of large particles / 4.4:
Planetesimal formation via coagulation / 4.5:
Coagulation equation / 4.5.1:
Sticking efficiencies / 4.5.2:
Goldreich-Ward mechanism / 4.6:
Gravitational stability of a particle layer / 4.6.1:
Application to planetesimal formation / 4.6.2:
Self-excited turbulence / 4.6.3:
Routes to planetesimal formation / 4.7:
Terrestrial planet formation / 4.8:
Physics of collisions / 5.1:
Gravitational focusing / 5.1.1:
Shear versus dispersion dominated encounters / 5.1.2:
Accretion versus disruption / 5.1.3:
Statistical models of planetary growth / 5.2:
Approximate treatment / 5.2.1:
Shear and dispersion dominated limits / 5.2.2:
Isolation mass / 5.2.3:
Velocity dispersion / 5.3:
Viscous stirring / 5.3.1:
Dynamical friction / 5.3.2:
Gas drag / 5.3.3:
Analytic formulae for planetary growth / 5.4:
Collisional damping and turbulent excitation / 5.5:
Final assembly / 5.6:
Giant planet formation / 5.8:
Core accretion / 6.1:
Core/envelope structure / 6.1.1:
Critical core mass / 6.1.2:
Growth of giant planets / 6.1.3:
Disk instability / 6.2:
Fragmentation conditions / 6.2.1:
Disk cooling time scale / 6.2.2:
Comparison with observations / 6.3:
Early evolution of planetary systems / 6.4:
Migration in gaseous disks / 7.1:
Resonant torques / 7.1.1:
Type 1 migration / 7.1.2:
Type 2 migration / 7.1.3:
Applications / 7.1.4:
Resonant evolution / 7.2:
Resonant capture / 7.2.1:
Kozai resonance / 7.2.2:
Migration in planetesimal disks / 7.3:
Application to the outer Solar System / 7.3.1:
The Nice Model / 7.3.2:
Application to extrasolar planetary systems / 7.3.3:
Planetary system stability / 7.4:
Hill stability / 7.4.1:
Planet-planet scattering / 7.4.2:
Physical and astronomical constants / 7.5:
N-body methods / Appendix 2:
References
Index
Preface
Observations of planetary systems / 1:
Solar System planets / 1.1:
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