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GAIA AND PHYSICS OF STELLAR INTERIORS
EAS Publications Series, 2002Understanding the stellar interiors is an important issue for astrophysics, but also for fundamental physics. The physical description of the stellar material implies statistical physics as well as hydrodynamics. We give examples of unsolved physical problems and their consequences for predictions of stellar properties and evolution.
Lebreton, Yveline, Baglin, Annie
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Physically realizable relativistic stellar structures
Astrophysics and Space Science, 1984Relativistic stellar structures can be obtained both analytically and by computation, but all these models do not stand the tests of physical reality. It is shown that for a physically reasonable solution dρ/dr ∝-r and d(e v /dr ∝r near the centre, d(P/ρ)/dr -(P/ρ).
M. C. Durgapal +2 more
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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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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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Stellar Spots — Physical Implications
1981Studies 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 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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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 Interiors
Physics Bulletin, 1975V C Reddish Edinburgh: Edinburgh University Press 1974 pp vii + 107 price £3 Written at an undergraduate/postgraduate level, this book is based on a course of lectures given by Dr Reddish to astronomy students at the Case-Western Reserve University, Cleveland, Ohio, in the spring of 1969. Part one of the book deals with the structure, energy generating
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Stellar Physics and Starburst Evolution
1998Starbursts regions offer a very interesting opportunity to study the links between stellar and galactic evolutions. Indeed starburst triggering is often related to dynamical processes. As mentioned in F. Combes’ lectures, the most spectacular starbursts occur in tidally interacting galaxies and mergers. On the other hand, many observational features of
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