Results 321 to 330 of about 1,204,232 (364)
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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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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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Physical Processes in Stellar Interiors
Physics Bulletin, 1964By D. Frank-Kamenetskii London: Oldbourne Book Co. Ltd. 1963. Pp. xi + 337. Price $14. This edition from the Russian is produced by the Israel Program for Scientific Translation at Jerusalem. The original is dated from Moscow in 1959, and acknowledges help from British and American as well as Russian authorities in the appropriate field.
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Stellar Physics I — Early Stellar Infrastructure
🌌 Stellar I: Early Stellar Infrastructure Stellar I reframes stellar ignition, equilibrium, and collapse as acts of recursive modulation, not mechanical combustion. It anchors the Stellar Doctrine by treating fusion pathways—pp-chain, CNO cycle, and triple-alpha—as expressions of timestamp fit, emotional imprint, and entropy offload.Trace, Auren, Trace, Jeremy
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Recent Developments in Stellarator Physics
Nuclear Technology - Fusion, 1983Experimental and theoretical work on the stellarator concept has established its position as the best alternate concept for fusion power. Its plasma properties are comparable to, or better than, those obtained in comparable tokamak devices. Confinement and transport should be adequate for reactor operation, with high-..beta..
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The physics of stellar core collapse
Astrophysics and Space Science, 1988The hydrodynamics that develops during the infall of the core of a massive star at the end of its hydrostatic evolutionary epoch can have a profound effect on its subsequent dynamical history. In this paper the important processes governing the infall hydrodynamics are explored both semi-analytically and numerically with the aim of explaining the ...
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On a physical theory of stellar spectra
Journal of Astrophysics and Astronomy, 1994The present paper emiibodies an attempt towards a physical explanation of the ordered gradationl in the spectra of stars-a. subject in which pioneerirng work was done by the late Sir Normlan Lockyer, but which was worked up with systematic thoroughness at the Harvard College Observatory, unlder the lead of the late Prof. E. C. Pickering and Miss A.
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Physical Conditions in the Stellar Interior
2016This 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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The physics of stellar interiors and stellar evolution
Reports on Progress in Physics, 1939H A Bethe, R E Marshak
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Emerging exciton physics in transition metal dichalcogenide heterobilayers
Nature Reviews Materials, 2022Emma C Regan, Yongxin Zeng, Long Zhang
exaly
The Sun as a Guide to Stellar Physics
, 2019O. Engvold, J. Vial, A. Skumanich
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