Leseprobe
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Theory of Stellar Atmospheres
Dimitri Mihalas, Ivan Hubeny
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Naturwissenschaften, Medizin, Informatik, Technik / Naturwissenschaften allgemein
Beschreibung
The most authoritative synthesis of the quantitative spectroscopic analysis of stellar atmospheres
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
Kundenbewertungen
Quantum superposition, Astronomical spectroscopy, Spin–orbit interaction, Plasma (physics), Gamma ray, Stellar evolution, Fermion, Atmosphere of Earth, Active galactic nucleus, Stellar parallax, Thermonuclear fusion, Einstein relation (kinetic theory), Substellar object, Galaxy rotation curve, Elliptic orbit, Solar mass, Spectral line, Intensity (physics), Stellar structure, Planetary science, Radiation, Scattering, Planetary nebula, Compton scattering, Galactic astronomy, Ionization, Hyades (star cluster), Neutrino, Spherical model, Astrophysics, Perturbation theory (quantum mechanics), Einstein coefficients, Nuclear density, Radiation damping, Solar luminosity, Celestial mechanics, Radiative transfer, Electron magnetic moment, Atomic nucleus, Fusion power, Synchrotron radiation, Temperature, Dirac equation, Stellar wind, Fermi–Dirac statistics, Photon, Conjunction (astronomy), Quantum mechanics, Calculation, Variational method (quantum mechanics), Radiation pressure, Spectroscopic notation, Neutrino detector, Chromosphere, Stellar classification, Ionization energy, Atomic theory, Optical depth, Maxwell–Boltzmann distribution, Orbital plane (astronomy), Relativistic quantum mechanics, Probability, Stellar atmosphere, Nuclear fusion, Emission spectrum, Kinetic theory of gases, Stellar mass, S-type star, Lorentz transformation, Thermodynamic equilibrium