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1.

図書

図書
edited by Bodo L. Ziegler ... [et al.]
出版情報: Cambridge : Cambridge University Press, 2014  xxix, 375 p. ; 26 cm
シリーズ名: IAU Symposium and Colloquium proceedings series ; 309
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2.

図書

図書
James Binney and Scott Tremaine
出版情報: Princeton, N.J. : Princeton University Press, c1987  xv, 733 p. ; 24 cm
シリーズ名: Princeton series in astrophysics
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3.

図書

図書
edited by Gerry Gilmore and Bob Carswell
出版情報: Dordrecht ; Tokyo : D. Reidel Pub. Co. , Norwell, MA : Sold and distributed in the U.S.A. and Canada by Kluwer Academic Publishers, c1987  xiii, 435 p. ; 25 cm
シリーズ名: NATO ASI series ; ser. C . Mathematical and physical sciences ; v. 207
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4.

図書

図書
William C. Saslaw
出版情報: Cambridge [Cambridgeshire] ; New York : Cambridge University Press, 1985  xvii, 491 p. ; 26 cm
シリーズ名: Cambridge monographs on mathematical physics
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Preface
Introduction
Idealized homogeneous systems - basic ideas and gentle relaxation / 1:
Infnite inhomogeneous systems - galaxy clustering / 2:
Finite spherical systems - cluster of galaxies, galactic nuclei, globular clusters / 3:
Finite flattered systems - galaxies / 4:
Index
Preface
Introduction
Idealized homogeneous systems - basic ideas and gentle relaxation / 1:
5.

図書

図書
H. Scheffler, H. Elsässer ; translated by A.H. Armstrong
出版情報: Berlin ; Tokyo : Springer-Verlag, c1987  xi, 492 p. ; 25 cm
シリーズ名: Astronomy and astrophysics library
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6.

図書

図書
by P.J.E. Peebles
出版情報: Princeton, N.J. : Princeton University Press, c1980  xiii, 422 p. ; 24 cm
シリーズ名: Princeton series in physics
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Preface
Acknowledgments
Homogeneity and Clustering / I.:
Homogeneity and clustering / 1.:
Is the universe homogeneous? / 2.:
Physical principles / 3.:
How did galaxies and clusters of galaxies form? / 4.:
Summary / 5.:
Behavior of Irregularities in the Distribution of Matter: Newtonian Approximation / II.:
Newtonian approximation / 6.:
Particle dynamics in expanding coordinates / 7.:
The peculiar acceleration / 8.:
Two models: the Vlasov equation and the ideal fluid / 9.:
Linear perturbation approximation for [delta] / 10.:
Solutions for [delta](t): p = [Lambda] = 0 / 11.:
Solutions for [delta](t): effect of a uniform radiation background / 12.:
Solutions for [delta](t): models with [Lambda not equal] 0 / 13.:
The peculiar velocity field / 14.:
Joining conditions for [delta] and [upsilon] / 15.:
Critical Jeans length / 16.:
Primeval magnetic field as a source for [delta rho] / [rho] / 17.:
Second order perturbation theory for [delta rho] / [rho] / 18.:
Spherical model / 19.:
Homogeneous ellipsoid model / 20.:
Caustics and pancakes / 21.:
Expansion, vorticity, and shear / 22.:
Origin of the rotation of galaxies / 23.:
Cosmic energy equation / 24.:
Spherical accretion model / 25.:
Hierarchical clustering model / 26.:
Fourier transform of the equations of motion / 27.:
Coupling of density fluctuations / 28.:
n-Point Correlation Functions: Descriptive Statistics / III.:
Statistical measures of the galaxy distribution / 29.:
Fair sample hypothesis / 30.:
Two-point spatial correlation function [xi](r) / 31.:
Two-point correlation function: another definition / 32.:
Two-point correlation function: Poisson model / 33.:
Three-point correlation function / 34.:
Four-point correlation function / 35.:
Moments of counts of objects / 36.:
Constraints on [xi] and [zeta] / 37.:
Probability generating function / 38.:
Estimates of P[subscript N] / 39.:
Cluster model / 40.:
Power spectrum / 41.:
Power law model for the spectrum / 42.:
Bispectrum / 43.:
Cross correlation function / 44.:
Angular two-point correlation function / 45.:
Angular power spectrum / 46.:
Estimating w([theta]) / 47.:
Statistical uncertainty in the estimate of w([theta]) / 48.:
Relation between angular and spatial two-point correlation functions / 49.:
Small separation approximation and the scaling relation / 50.:
Decoupling of magnitude and position / 51.:
Relation between [xi] and w: some examples / 52.:
Inversion of the equation / 53.:
Angular three-point correlation function / 54.:
Angular four-point correlation function / 55.:
Correction for curvature and expansion / 56.:
Summary of numerical results / 57.:
Power spectrum of the extragalactic light / 58.:
Moments of the number of neighbors / 59.:
Model for P[subscript N] / 60.:
Clustering models / 61.:
Continuous clustering hierarchy: Mandelbrot's prescription / 62.:
The mass correlation functions / 63.:
Clustering hierarchy: continuity speculation / 64.:
Remarks on the observations / 65.:
Dynamics and Statistics / IV.:
Goals / 66.:
Definitions of variables and distribution functions / 67.:
BBGKY hierarchy equations / 68.:
Fluid limit / 69.:
Evolution of the integral of [xi] / 70.:
Particle conservation equations / 71.:
Relative peculiar velocity dispersion / 72.:
Similarity solution / 73.:
Cosmic virial theorem / 74.:
Joint distribution in position and velocity / 76.:
Behavior of the halo around a cluster of galaxies / 77.:
Superclusters / 78.:
Problems and prospects / 79.:
Relativistic Theory of the Behavior of Irregularities in an Expanding World Model / V.:
Role of the relativistic theory / 80.:
Time-orthogonal coordinates / 81.:
The field equations for h[subscript alpha beta] / 82.:
Gravitational waves / 83.:
Linear perturbation equations for the matter / 84.:
Behavior of density perturbations at wavelength [characters not reproducible] ct / 86.:
Evolution of acoustic waves / 87.:
Nonlinear acoustic waves / 89.:
Incompressible flow / 90.:
Behavior of collisionless particles / 91.:
Linear dissipation of adiabatic perturbations / 92.:
Residual fluctuations in the microwave background / 93.:
Isothermal perturbations / 94.:
Scenarios / VI.:
Nature of the universe at high redshift / 95.:
Nature of protogalaxies and protoclusters / 96.:
Appendix
Models and notation / 97.:
List of Abbreviations
References
Index
Preface
Acknowledgments
Homogeneity and Clustering / I.:
7.

図書

図書
James Binney and Michael Merrifield
出版情報: Princeton, N.J. : Princeton University Press, 1998  xiii, 796 p. ; 24 cm
シリーズ名: Princeton series in astrophysics
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Preface
Galaxies: an overview
Introduction / 1.1:
A brief history of galactic astronomy / 1.2:
Photometric models of the Milky Way
The nature of the spiral nebulae
Kinematic models of the Milky Way
Stellar populations
More recent developments
Positions, motions and coordinate systems / 2.1:
The equatorial system
Galactic coordinates
Parallax
Proper motions
Precession and nutation
Astrometric systems
Distances determined from velocities / 2.2:
Radial velocities
Distances from the movingcluster method
Secular parallaxes
Statistical parallaxes
Magnitudes and colors / 2.3:
Apparent magnitudes
Colors
Absolute magnitudes
Absolute energy distributions
and bolometric magnitudes
Mass-to-light ratios
Surface brightness and isophotal radii
Gravitational lensing / 2.4:
Archival data and catalogs / 2.5:
On-line resources
Problems
The masses of stars / 3.1:
The Mass of the Sun
Masses of binary stars
Visual binaries
Spectroscopic binaries
The radii of stars / 3.2:
Phase interferometry
Intensity interferometry
Speckle interferometry
Lunar occultations
Eclipsing binaries
Astrophysical estimates
Classification of stars / 3.3:
Novae
Pulsars
Classification of stellar spectra
The MK system
Physical interpretation of stellar spectra / 3.4:
Color-magnitude diagrams / 3.5:
Observed Cm-diagrams
Luminosity and color as functions of spectral class
The physical properties of stars on the MS and RGB
The stellar luminosity function / 3.6:
Malmquist bias
Lutz-Kelker Bias
The general luminosity function
Cluster luminosity functions
Photometrically complete surveys
Proper-motion selected surveys
The luminosity function of a given MK spectral class
Catalogs of the nearby stars
Interstellar dust / 3.7:
Extinction and reddening
Reddening-free indices
Polarization of starlight by dust
Extinction of sightlines out of the Galaxy
Morphological classification of galaxies / 4.1:
The Hubble sequence
Effects of environment
The galaxy luminosity function
The field galaxy luminosity function
The cluster galaxy luminosity function
The luminosity function divided by morphological type
The Local Group
Surface Photometry of Galaxies / 4.2:
The night sky
Effect of seeing
Deprojecting galaxy images
Photometry of Elliptical Galaxies / 4.3:
Radial surface-brightness profiles of elliptical galaxies
Preface
Galaxies: an overview
Introduction / 1.1:
8.

電子ブック

EB
John Gribbin
出版情報: Oxford : Oxford University Press, 2008  1 online resource (121 p.)
シリーズ名: Very short introductions ; 182
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9.

図書

図書
James Binney and Scott Tremaine
出版情報: Princeton, N.J. : Princeton University Press, c2008  xvi, 885 p., [16] p. of plates ; 24 cm
シリーズ名: Princeton series in astrophysics
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Preface
Introduction / Chapter 1:
An overview of the observations / 1.1:
Collisionless systems and the relaxation time / 1.2:
The relaxation time
The cosmological context / 1.3:
Potential Theory / Chapter 2:
General results / 2.1:
The potential-energy tensor
Spherical systems / 2.2:
Potential-density pairs for attened systems / 2.3:
Multipole expansion / 2.4:
The potentials of spheroidal and ellipsoidal systems / 2.5:
The potentials of disks / 2.6:
The potential of our Galaxy / 2.7:
Potentials from functional expansions / 2.8:
Poisson solvers for N-body codes / 2.9:
The Orbits of Stars / Chapter 3:
Orbits in static spherical potentials / 3.1:
Orbits in axisymmetric potentials / 3.2:
Orbits in planar non-axisymmetric potentials / 3.3:
Numerical orbit integration / 3.4:
Angle-action variables / 3.5:
Slowly varying potentials / 3.6:
Perturbations and chaos / 3.7:
Orbits in elliptical galaxies / 3.8:
Equilibria of Collisionless Systems / Chapter 4:
The collisionless Boltzmann equation / 4.1:
Jeans theorems / 4.2:
DFs for spherical systems / 4.3:
DFs for axisymmetric density distributions / 4.4:
DFs for razor-thin disks / 4.5:
Using actions as arguments of the DF / 4.6:
Particle-based and orbit-based models / 4.7:
The Jeans and virial equations / 4.8:
Stellar kinematics as a mass detector / 4.9:
The choice of equilibrium / 4.10:
Stability of Collisionless Systems / Chapter 5:
The response of homogeneous systems / 5.1:
General theory of the response of stellar systems / 5.3:
The energy principle and secular stability / 5.4:
The response of spherical systems / 5.5:
The stability of uniformly rotating systems / 5.6:
Disk Dynamics and Spiral Structure / Chapter 6:
Fundamentals of spiral structure / 6.1:
Wave mechanics of differentially rotating disks / 6.2:
Global stability of differentially rotating disks / 6.3:
Damping and excitation of spiral structure / 6.4:
Bars / 6.5:
Warping and buckling of disks / 6.6:
Kinetic Theory / Chapter 7:
Relaxation processes / 7.1:
The thermodynamics of self-gravitating systems / 7.2:
The Fokker Planck approximation / 7.4:
The evolution of spherical stellar systems / 7.5:
Summary / 7.6:
Collisions and Encounters of Stellar Systems / Chapter 8:
Dynamical friction / 8.1:
High-speed encounters / 8.2:
Tides / 8.3:
Encounters in stellar disks / 8.4:
Mergers / 8.5:
Galaxy Formation / Chapter 9:
Linear structure formation / 9.1:
Nonlinear structure formation / 9.2:
N-body simulations of clustering / 9.3:
Star formation and feedback / 9.4:
Conclusions / 9.5:
Useful numbers / Appendices A:
Mathematical background / B:
Special functions / C:
Mechanics / D:
Delaunay variables for Kepler orbits / E:
Fluid mechanics / F:
Discrete Fourier transforms / G:
The Antonov Lebovitz theorem / H:
The Doremus Feix Baumann theorem / I:
Angular-momentum transport in disks / J:
Derivation of the reduction factor / K:
The diffusion coefficients / L:
The distribution of binary energies / M:
References
Index
Stars / 1:
The Galaxy
Other galaxies
Elliptical galaxies
Spiral galaxies
Lenticular galaxies
Irregular galaxies
Open and globular clusters
Groups and clusters of galaxies
Black holes
Kinematics
Geometry
Dynamics
The Big Bang and inflation
The cosmic microwave background
Problems
Newton's theorems / 2:
Potential energy of spherical systems
Potentials of some simple systems
Point mass
Homogeneous sphere
Plummer model
Isochrone potential
Modified Hubble model
Power-law density model
Two-power density models
Potential-density pairs for flattened systems
Kuzmin models and generalizations
Logarithmic potentials
Poisson's equation in very flattened systems
Potentials of spheroidal shells
Potentials of spheroidal systems
Potentials of ellipsoidal systems
Ferrers potentials
Potential-energy tensors of ellipsoidal systems
Disk potentials from homoeoids
The Mestel disk
The exponential disk
Thick disks
Disk potentials from Bessel functions
Application to axisymmetric disks
Disk potentials from logarithmic spirals
Disk potentials from oblate spheroidal coordinates
The bulge
The dark halo
The stellar disk
The interstellar medium
The bulge as a bar
Bi-orthonormal basis functions
Designer basis functions
Direct summation
Softening
Tree codes
Cartesian multipole expansion
Particle-mesh codes
Periodic boundary conditions
Vacuum boundary conditions
Mesh refinement
P[superscript 3]M codes
Spherical-harmonic codes
Simulations of planar systems
Spherical harmonic oscillator / 3:
Kepler potential
Hyperbolic encounters
Constants and integrals of the motion
Motion in the meridional plane
Surfaces of section
Nearly circular orbits: epicycles and the velocity ellipsoid
Two-dimensional non-rotating potential
Two-dimensional rotating potential
Weak bars
Lindblad resonances
Orbits trapped at resonance
Symplectic integrators
Modified Euler integrator
Leapfrog integrator
Runge-Kutta and Bulirsch-Stoer integrators
Multistep predictor-corrector integrators
Multivalue integrators
Adaptive timesteps
Individual timesteps
Regularization
Burdet-Heggie regularization
Kustaanheimo-Stiefel (KS) regularization
Orbital tori
Time averages theorem
Action space
Hamilton-Jacobi equation
Angle-action variables for spherical potentials
Angle-action variables for flattened axisymmetric potentials
Stackel potentials
Epicycle approximation
Angle-action variables for a non-rotating bar
Adiabatic invariance of actions
Applications
Harmonic oscillator
Eccentric orbits in a disk
Transient perturbations
Slow growth of a central black hole
Hamiltonian perturbation theory
Trapping by resonances
Levitation
From order to chaos
Irregular orbits
Frequency analysis
Liapunov exponents
The perfect ellipsoid
Dynamical effects of cusps
Dynamical effects of black holes
Limitations of the collisionless Boltzmann equation / 4:
Finite stellar lifetimes
Correlations between stars
Relation between the DF and observables
An example
Choice of f and relations between moments
DF depending only on H
DF depending on H and L
DF depending on H and L[subscript z]
Ergodic DFs for systems
Ergodic Hernquist, Jaffe and isochrone models
Differential energy distribution
DFs for anisotropic spherical systems
Models with constant anisotropy
Osipkov-Merritt models
Other anisotropic models
Differential-energy distribution for anisotropic systems
Spherical systems defined by the DF
Polytropes and the Plummer model
The isothermal sphere
Lowered isothermal models
Double-power models
Michie models
DF for a given axisymmetric system
Axisymmetric systems specified by f(H, L[subscript z])
Fully analytic models
Rowley models
Rotation and flattening in spheroids
The Schwarzschild DF
Mestel disk
Kalnajs disks
Adiabatic compression
Cusp around a black hole
Adiabatic deformation of dark matter
N-body modeling
Instability and chaos
Schwarzschild models
Jeans equations for spherical systems
Effect of a central black hole on the observed velocity dispersion
Jeans equations for axisymmetric systems
Asymmetric drift
Spheroidal components with isotropic velocity dispersion
Virial equations
Scalar virial theorem
The tensor virial theorem and observational data
Detecting black holes
Extended mass distributions of elliptical galaxies
Dynamics of the solar neighborhood
The principle of maximum entropy
Phase mixing and violent relaxation
Phase mixing
Violent relaxation
Numerical simulation of the relaxation process
Linear response theory / 5:
Linearized equations for stellar and fluid systems
Physical basis of the Jeans instability
Homogeneous systems and the Jeans swindle
The response of a homogeneous fluid system
The response of a homogeneous stellar system
Unstable solutions
Neutrally stable solutions
Damped solutions
Discussion
The polarization function in angle-action variables
The Kalnajs matrix method
The response matrix
The energy principle for fluid systems
The energy principle for stellar systems
The relation between the stability of fluid and stellar systems
The stability of spherical systems with ergodic DFs
The stability of anisotropic spherical systems
Physical basis of the radial-orbit instability
Landau damping and resonances in spherical systems
The uniformly rotating sheet
Maclaurin spheroids and disks
Images of spiral galaxies / 6:
Spiral arms at other wavelengths
Dust
Relativistic electrons
Molecular gas
Neutral atomic gas
HII regions
The geometry of spiral arms
The strength and number of arms
Leading and trailing arms
The pitch angle and the winding problem
The pattern speed
The anti-spiral theorem
Angular-momentum transport by spiral-arm torques
Preliminaries
Kinematic density waves
Resonances
The dispersion relation for tightly wound spiral arms
The tight-winding approximation
Potential of a tightly wound spiral pattern
The dispersion relation for fluid disks
The dispersion relation for stellar disks
Local stability of differentially rotating disks
Long and short waves
Group velocity
Energy and angular momentum in spiral waves
Numerical work on disk stability
Swing amplifier and feedback loops
The swing amplifier
Feedback loops
Physical interpretation of the bar instability
The maximum-disk hypothesis
Response of the interstellar gas to a density wave
Response of a density wave to the interstellar gas
Excitation of spiral structure
Excitation by companion galaxies
Excitation by bars
Stationary spiral structure
Excitation of intermediate-scale structure
Observations
Dynamics of bars
Strong bars
The vertical structure of bars
Gas flow in bars
Slow evolution of bars
Warps
Kinematics of warps
Bending waves with self-gravity
The origin of warps
Buckling instability
Relaxation / 7:
Equipartition
Escape
Inelastic encounters
Binary formation by triple encounters
Interactions with primordial binaries
Virial theorem
Liouville's theorem
Reduced distribution functions
Relation of Liouville's equation to the collisionless Boltzmann equation
Negative heat capacity
The gravothermal catastrophe
The Fokker-Planck approximation
The master equation
Fokker-Planck equation
Weak encounters
Local encounters
Orbit-averaging
Fluctuation-dissipation theorems
Diffusion coefficients
Heating of the Galactic disk by MACHOs
Relaxation time
Numerical methods
Fluid models
Monte Carlo methods
Numerical solution of the Fokker-Planck equation
N-body integrations
Checks and comparisons
Mass loss from stellar evolution
Evaporation and ejection
The maximum lifetime of a stellar system
Core collapse
After core collapse
Tidal shocks and the survival of globular clusters
Binary stars
Soft binaries
Hard binaries
Reaction rates
Stellar systems with a central black hole
Consumption of stars by the black hole
The effect of a central black hole on the surrounding stellar system
The validity of Chandrasekhar's formula / 8:
Applications of dynamical friction
Decay of black-hole orbits
Galactic cannibalism
Orbital decay of the Magellanic Clouds
Dynamical friction on bars
Formation and evolution of binary black holes
Globular clusters
Mass loss
Return to equilibrium
Adiabatic invariance
The distant-tide approximation
Disruption of stellar systems by high-speed encounters
The catastrophic regime
The diffusive regime
Disruption of open clusters
Disruption of binary stars
Dynamical constraints on MACHOs
Disk and bulge shocks
High-speed interactions in clusters of galaxies
The restricted three-body problem
The sheared-sheet or Hill's approximation
The epicycle approximation and Hill's approximation
The Jacobi radius in Hill's approximation
Tidal tails and streamers
Scattering of disk stars by molecular clouds
Scattering of disk stars by spiral arms
Peculiar galaxies
Grand-design spirals
Ring galaxies
Shells and other fine structure
Starbursts
The merger rate
Gaussian random fields / 9:
Filtering
The Harrison-Zeldovich power spectrum
Gravitational instability in the expanding universe
Non-relativistic fluid
Relativistic fluid
Spherical collapse
The cosmic web
Press-Schechter theory
The mass function
Collapse and virialization in the cosmic web
The mass function of halos
Radial density profiles
Internal dynamics of halos
The shapes of halos
Rotation of halos
Dynamics of halo substructure
Reionization
Feedback
Mergers, starbursts and quiescent accretion
The role of central black holes
Origin of the galaxy luminosity function
Appendices
Vectors / A:
Curvilinear coordinate systems
Vector calculus
Fourier series and transforms
Abel integral equation
Schwarz's inequality
Calculus of variations
Poisson distribution
Conditional probability and Bayes's theorem
Central limit theorem
Delta function and step function
Factorial or gamma function
Error function, Dawson's integral, and plasma dispersion function
Elliptic integrals
Legendre functions
Spherical harmonics
Bessel functions
Single particles
Systems of particles
Lagrangian dynamics
Hamiltonian dynamics
Hamilton's equations
Poincare invariants
Poisson brackets
Canonical coordinates and transformations
Extended phase space
Generating functions
Basic equations
Continuity equation
Euler's equation
Energy equation
Equation of state
The ideal gas
Sound waves
Energy and momentum in sound waves
The Antonov-Lebovitz theorem
The Doremus-Feix-Baumann theorem
Transport in fluid and stellar systems
Transport in a disk with stationary spiral structure
Transport in perturbed axisymmetric disks
Transport in the WKB approximation
The evolution of the energy distribution of binaries
The two-body distribution function in thermal equilibrium
The distribution of binary energies in thermal equilibrium
The principle of detailed balance
Preface
Introduction / Chapter 1:
An overview of the observations / 1.1:
10.

図書

図書
Flügge, Siegfried
出版情報: Berlin : Springer-Verlag, 1959  viii, 565 p. ; 26 cm
シリーズ名: Handbuch der Physik / herausgegeben von S. Flügge = Encyclopedia of physics / editor in chief, S. Flügge ; Bd. 53 . Astrophysik = Astrophysics ; 4
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