Results 301 to 310 of about 985,930 (333)

Stellar Clusters: Benchmarks of Stellar Physics and Galactic Evolution - EES2015

2016
Not ...
Moraux, Estelle, Lebreton, Yveline, Charbonnel, Corinne   +2 more
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Physics at the stellarator--tokamak interface

Plasma Physics and Controlled Fusion, 2011
A tokamak is never exactly axisymmetric, either because of field errors or because the magnetic field is intentionally perturbed–something that is becoming increasingly popular for controlling the plasma edge. Conversely, a stellarator generally lacks symmetry but may be `quasisymmetric', meaning that the strength (but not the direction) of the ...
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Stellar Evolution Physics

2012
This volume explains the microscopic physics operating in stars in advanced stages of their evolution and describes with many numerical examples and illustrations how they respond to this microphysics. Models of low and intermediate mass are evolved through the core helium-burning phase, the asymptotic giant branch phase (alternating shell hydrogen and
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Stellar Spots — Physical Implications [PDF]

, 1981
Studies of certain late-type stars have revealed evidence for appreciable changes in their photospheric radiation. These stars are rotating much more rapidly than the Sun and/or are younger, and exhibit much enhanced examples of many kinds of solar activity, such as flares.
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Physical mechanisms in stellar pulsations

The Journal of the Acoustical Society of America, 1985
Stars evolve from their births to their deaths by converting their store of hydrogen to helium, and then much of this helium is fused to heavier elements such as carbon, oxygen, and up to iron. During this evolution, the stellar mass may decrease by a stellar wind mass loss, the radius usually greatly increases, and the radiation luminosity emitted at ...
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The physics of stellar interiors and stellar evolution

Reports on Progress in Physics, 1939
Hans A. Bethe, Robert E. Marshak
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Physical Conditions in the Stellar Interior

2016
This chapter establishes the main equations of the stellar structure, namely, the continuity equation and the hydrostatic equilibrium equation, and gives some estimates of the average density, pressure, and temperature. Finally, a discussion is made of the thermodynamic equilibrium and the stellar energy.
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Physics-informed machine learning

Nature Reviews Physics, 2021
George Em Karniadakis, Weiliang Xia, Liu Yang   +2 more
exaly  

Stellar Evolution Physics – Volume 1. Physical Processes in Stellar Interiors

, 2016
B. Ishak
semanticscholar   +1 more source

Doping a Mott insulator: Physics of high-temperature superconductivity

Reviews of Modern Physics, 2006
Xiao-gang Wen
exaly