Science · 1994 · 188 citations · 37 references
Natural SciencesAstronomyPhysicsAstrophysicsCosmologyRadiation TransportNuclear AstrophysicsRadiative ProcessesRadiative TransferStellar AstrophysicsStellar EvolutionStellar StructureAstrophysical Photon TransportEnergy Transport In StarsEquation Of State Of Stellar MatterOpacity CalculationsOpacity ModelingRadiative Thermal PropertiesRadiative Transfer In Stellar EnvelopesStellar Opacities
An array of problems in astronomy, cosmology, and particle physics is dependent on our understanding of the evolution and structure of stars. Stellar structure and evolution, in turn, depend on how the nuclear energy generated in the stellar center is transported to the surface. Energy transport by photons is a primary transfer mechanism. Recent improvements in the calculation of the radiative properties of stellar matter have helped resolve several long-standing discrepancies between observations and the predictions of theoretical models.
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Solar models, neutrino experiments, and helioseismology
John N. Bahcall, R. K. Ulrich · Reviews of Modern Physics · 1988 · 898 citations
Natural Sciences, Astronomy, Physics +15
Opacities for stellar envelopes
M. J. Seaton, Yu Yan, Dimitri Mihalas et al. · Monthly Notices of the Royal Astronomical Society · 1994 · 608 citations · Full text