Dynamical Evolution of Globular Clusters

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A01=Jr.
A01=Lyman Spitzer
Acceleration
Accretion (astrophysics)
Adiabatic invariant
Age Group_Uncategorized
Age Group_Uncategorized
Angular frequency
Angular momentum
Approximation
Asymptotic expansion
Author_Jr.
Author_Lyman Spitzer
Autocorrelation
automatic-update
Binary star
Boltzmann equation
Calculation
Category1=Non-Fiction
Category=PHVB
Category=PSAJ
Center of mass (relativistic)
Circular orbit
Cluster expansion
Computation
COP=United States
Cross section (physics)
Delivery_Pre-order
Distribution function
Dynamical friction
Dynamical time scale
Elliptic orbit
eq_isMigrated=2
eq_non-fiction
eq_science
Equation
Equipartition theorem
Equipotential
Escape velocity
Fokker–Planck equation
Galactic Center
Galactic halo
Galactic plane
Giant star
Globular cluster
Gravitational acceleration
Gravitational collapse
Gravitational constant
Gravitational energy
Gravitational field
Gravitational potential
Gravity
Hertzsprung–Russell diagram
Impact parameter
Instability
Jr.
Kinetic energy
Language_English
Luminosity
Main sequence
Mass diffusivity
Mass distribution
Maxwell–Boltzmann distribution
Metallicity
Molecular cloud
Monte Carlo method
Neutron star
Orbit
Orbital elements
Orbital period
Order of magnitude
PA=Temporarily unavailable
Phase space
Price_€50 to €100
Probability
PS=Active
Quantity
Relative velocity
Renormalization
Resonance
Semi-major and semi-minor axes
Series expansion
softlaunch
Spherical model
Stellar collision
Stellar dynamics
Stellar evolution
Stellar mass
Tidal force
Velocity dispersion
Virial theorem

Product details

  • ISBN 9780691635361
  • Weight: 539g
  • Dimensions: 178 x 254mm
  • Publication Date: 19 Apr 2016
  • Publisher: Princeton University Press
  • Publication City/Country: US
  • Product Form: Hardback
  • Language: English
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One of the world's most distinguished astrophysicists presents a comprehensive theoretical treatment of the dynamical evolution of globular clusters. Lyman Spitzer's research in this field established the framework for decades of investigation. Now he summarizes in a unified, systematic way this branch of theoretical astrophysics with its still challenging problems. Originally published in 1988. The Princeton Legacy Library uses the latest print-on-demand technology to again make available previously out-of-print books from the distinguished backlist of Princeton University Press. These editions preserve the original texts of these important books while presenting them in durable paperback and hardcover editions. The goal of the Princeton Legacy Library is to vastly increase access to the rich scholarly heritage found in the thousands of books published by Princeton University Press since its founding in 1905.