Structure and Evolution of Stars

Regular price €67.99
Quantity:
Ships in 10-20 days
Delivery/Collection within 10-20 working days
Shipping & Delivery
A01=Martin Schwarzschild
Accretion (astrophysics)
Age Group_Uncategorized
Age Group_Uncategorized
Alpha particle
Astronomer
Astronomical spectroscopy
Astronomy
Astrophysics
Atomic absorption spectroscopy
Atomic number
Author_Martin Schwarzschild
automatic-update
Be star
Binary star
Carbon star
Category1=Non-Fiction
Category=PGM
Category=PHVB
Celestial mechanics
Chromosphere
Conjunction (astronomy)
Convection
Convection zone
COP=United States
Delivery_Delivery within 10-20 working days
Elliptical galaxy
eq_bestseller
eq_isMigrated=2
eq_nobargain
eq_non-fiction
eq_science
Equation of state
Equation of state (cosmology)
Formation and evolution of the Solar System
Galactic plane
Galaxy rotation curve
Gamma ray
Globular cluster
Gravitational energy
Gravitational potential
Hertzsprung-Russell diagram
Hyades (star cluster)
Interstellar cloud
Interstellar medium
Kepler's laws of planetary motion
Language_English
Luminosity
Luminosity function (astronomy)
Main sequence
Neutrino
Nuclear density
Nuclear reaction
Observational astronomy
Orbit
Orbital eccentricity
Orbital period
PA=Available
Perturbation theory (quantum mechanics)
Photon
Planetary nebula
Positron
Price_€50 to €100
Proton-proton chain reaction
PS=Active
Quantity
Radiation flux
Radiation pressure
Red giant
RR Lyrae variable
softlaunch
Solar luminosity
Solar mass
Solar radius
Star
Star cluster
Star formation
Stellar atmosphere
Stellar evolution
Stellar kinematics
Stellar mass
Stellar population
Stellar pulsations
Stellar structure
Supergiant
Supernova
Temperature
Temperature gradient
Variable star
White dwarf

Product details

  • ISBN 9780691626598
  • Weight: 425g
  • Dimensions: 152 x 235mm
  • Publication Date: 08 Dec 2015
  • Publisher: Princeton University Press
  • Publication City/Country: US
  • Product Form: Paperback
  • Language: English
Secure checkout Fast Shipping Easy returns
With the development of nuclear physics the theory of the stellar interior entered a new phase. Many new investigations have been conducted and the results published in a variety of specialized media. This book brings these results together in a single volume and summarizes the present status of the theory of stellar evolution. Originally published in 1958. 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.

More from this author