Theory of Stellar Atmospheres
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★★★★★
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A01=Dimitri Mihalas
A01=Ivan Hubeny
Active galactic nucleus
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Age Group_Uncategorized
Astronomical spectroscopy
Astrophysics
Atmosphere of Earth
Atomic nucleus
Atomic theory
Author_Dimitri Mihalas
Author_Ivan Hubeny
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Calculation
Category1=Non-Fiction
Category=PHVB
Category=PNFS
Celestial mechanics
Chromosphere
Compton scattering
Conjunction (astronomy)
COP=United States
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Dirac equation
Einstein coefficients
Einstein relation (kinetic theory)
Electron magnetic moment
Elliptic orbit
Emission spectrum
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eq_non-fiction
eq_science
Fermion
Fermi–Dirac statistics
Fusion power
Galactic astronomy
Galaxy rotation curve
Gamma ray
Hyades (star cluster)
Intensity (physics)
Ionization
Ionization energy
Kinetic theory of gases
Language_English
Lorentz transformation
Maxwell–Boltzmann distribution
Neutrino
Neutrino detector
Nuclear density
Nuclear fusion
Optical depth
Orbital plane (astronomy)
PA=Available
Perturbation theory (quantum mechanics)
Photon
Planetary nebula
Planetary science
Plasma (physics)
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Probability
PS=Active
Quantum mechanics
Quantum superposition
Radiation
Radiation damping
Radiation pressure
Radiative transfer
Relativistic quantum mechanics
S-type star
Scattering
SN=Princeton Series in Astrophysics
softlaunch
Solar luminosity
Solar mass
Spectral line
Spectroscopic notation
Spherical model
Spin–orbit interaction
Stellar atmosphere
Stellar classification
Stellar evolution
Stellar mass
Stellar parallax
Stellar structure
Stellar wind
Substellar object
Synchrotron radiation
Temperature
Thermodynamic equilibrium
Thermonuclear fusion
Variational method (quantum mechanics)
Product details
- ISBN 9780691163291
- Weight: 1559g
- Dimensions: 152 x 235mm
- Publication Date: 26 Oct 2014
- Publisher: Princeton University Press
- Publication City/Country: US
- Product Form: Paperback
- Language: English
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This book provides an in-depth and self-contained treatment of the latest advances achieved in quantitative spectroscopic analyses of the observable outer layers of stars and similar objects. Written by two leading researchers in the field, it presents a comprehensive account of both the physical foundations and numerical methods of such analyses. The book is ideal for astronomers who want to acquire deeper insight into the physical foundations of the theory of stellar atmospheres, or who want to learn about modern computational techniques for treating radiative transfer in non-equilibrium situations. It can also serve as a rigorous yet accessible introduction to the discipline for graduate students. * Provides a comprehensive, up-to-date account of the field* Covers computational methods as well as the underlying physics* Serves as an ideal reference book for researchers and a rigorous yet accessible textbook for graduate students* An online illustration package is available to professors at press.princeton.edu
Ivan Hubeny is a senior research scientist at the Steward Observatory and adjunct professor in the Department of Astronomy at the University of Arizona. Dimitri Mihalas (1939-2013) was an astrophysicist at the Los Alamos National Laboratory. His many books include Stellar Atmospheres and Foundations of Radiation Hydrodynamics.
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