A01=Dimitri Mihalas

A01=Ivan Hubeny

Active galactic nucleus

Age Group_Uncategorized

Astronomical spectroscopy

Astrophysics

Atmosphere of Earth

Atomic nucleus

Atomic theory

Author_Dimitri Mihalas

Author_Ivan Hubeny

automatic-update

Calculation

Category1=Non-Fiction

Category=PHVB

Category=PNFS

Celestial mechanics

Chromosphere

Compton scattering

Conjunction (astronomy)

COP=United States

Delivery_Delivery within 10-20 working days

Dirac equation

Einstein coefficients

Einstein relation (kinetic theory)

Electron magnetic moment

Elliptic orbit

Emission spectrum

eq_isMigrated=2

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)

Price_€100 and above

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)

Theory of Stellar Atmospheres

Name: Theory of Stellar Atmospheres
Brand: Princeton University Press
SKU: 9780691163291
Price: 104.99 EUR
Availability: InStock

★★★★★

3.00 (1 ratings by Goodreads)

English

By (author): Dimitri Mihalas Ivan Hubeny

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 See more

€104.99

€105.99

Save 1%

Quantity

A01=Dimitri MihalasA01=Ivan HubenyActive galactic nucleusAge Group_UncategorizedAstronomical spectroscopyAstrophysicsAtmosphere of EarthAtomic nucleusAtomic theoryAuthor_Dimitri MihalasAuthor_Ivan Hubenyautomatic-updateCalculationCategory1=Non-FictionCategory=PHVBCategory=PNFSCelestial mechanicsChromosphereCompton scatteringConjunction (astronomy)COP=United StatesDelivery_Delivery within 10-20 working daysDirac equationEinstein coefficientsEinstein relation (kinetic theory)Electron magnetic momentElliptic orbitEmission spectrumeq_isMigrated=2eq_non-fictioneq_scienceFermionFermi–Dirac statisticsFusion powerGalactic astronomyGalaxy rotation curveGamma rayHyades (star cluster)Intensity (physics)IonizationIonization energyKinetic theory of gasesLanguage_EnglishLorentz transformationMaxwell–Boltzmann distributionNeutrinoNeutrino detectorNuclear densityNuclear fusionOptical depthOrbital plane (astronomy)PA=AvailablePerturbation theory (quantum mechanics)PhotonPlanetary nebulaPlanetary sciencePlasma (physics)Price_€100 and aboveProbabilityPS=ActiveQuantum mechanicsQuantum superpositionRadiationRadiation dampingRadiation pressureRadiative transferRelativistic quantum mechanicsS-type starScatteringSN=Princeton Series in AstrophysicssoftlaunchSolar luminositySolar massSpectral lineSpectroscopic notationSpherical modelSpin–orbit interactionStellar atmosphereStellar classificationStellar evolutionStellar massStellar parallaxStellar structureStellar windSubstellar objectSynchrotron radiationTemperatureThermodynamic equilibriumThermonuclear fusionVariational method (quantum mechanics)

Delivery/Collection within 10-20 working days

Product Details

Weight: 1559g
Dimensions: 152 x 235mm
Publication Date: 26 Oct 2014
Publisher: Princeton University Press
Publication City/Country: US
Language: English
ISBN13: 9780691163291

About Dimitri MihalasIvan Hubeny

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.