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High Energy Phenomena Around Collapsed Stars

ThlS volume contalns a serles of lectures presented at the NATO Advanced Study Instltute on Hlgh Energy Phenomena Around Collapsed Stars;

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Introduction to High-Energy Astrophysics

High-energy astrophysics covers cosmic phenomena that occur under the most extreme physical conditions. It explores the most violent events;

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Introduction to High-Energy Astrophysics

High-energy astrophysics covers cosmic phenomena that occur under the most extreme physical conditions. It explores the most violent events;

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High-Energy Astrophysics

High-energy astrophysics involves the study of exceedingly dynamic and energetic phenomena occurring near the most extreme celestial;

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Wolf-Rayet Stars

massive binary evolution; dust formation near WR stars and other circumstellar phenomena; and hydrodynamics and high-energy physics of colliding;

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Matter Under Extreme Conditions

, solar neutrinos, the physics of enormous densities and temperatures in stars and of immense magnetic fields around collapsed stars, strong;

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Foundations of High-Energy-Density Physics

High-energy-density physics explores the dynamics of matter at extreme conditions. This encompasses temperatures and densities far greater;

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High Energy Physics

The 32nd International Conference on High Energy Physics belongs to the Rochester Conference Series, and is the most important;

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High Energy Astrophysics

Providing students with an in-depth account of the astrophysics of high energy phenomena in the Universe, the third edition of this well;

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Extreme Environment Astrophysics

Covering host systems of accreting, relativistic bodies, and the high-energy phenomena associated with them, this self-contained;

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Extreme Environment Astrophysics

Covering host systems of accreting, relativistic bodies, and the high-energy phenomena associated with them, this self-contained;

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Elementary Lectures On Electric Discharges, Waves And Impulses, And Other Transients - Second Edition

Of Permanent Phenomena, Transients Existing With All Forms Of Energy, Destructive Values, High-Speed Water-Power Governing, Fundamental Condition;

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Cambridge Monographs on Particle Physics, Nuclear Physics and Cosmology

collisions, nuclear theory or high energy phenomenology, as well as astrophysicists interested in the phases of nuclear matter and its impact on;

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The Phases of Quantum Chromodynamics

collisions, nuclear theory or high energy phenomenology, as well as astrophysicists interested in the phases of nuclear matter and its impact on;

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Ferroelectrics

dielectric physics. Ferroelectric materials are important functional materials for various applications such as NVRAMs, high energy density;

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Atoms, Stars, and Nebulae

of stars is followed by an exploration of their interiors and how stars generate energy. An account of the exciting new field of high energy;

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Atoms, Stars, and Nebulae

of stars is followed by an exploration of their interiors and how stars generate energy. An account of the exciting new field of high energy;

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Multiwavelength Approach to Unidentified Gamma-Ray Sources

attempts at identifying them. To establish the origin and nature of these enigmatic sources has become a major problem of current high-energy;

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Heavy Ion Collisions At Intermediate Energy

with low energy, intermediate energy, high energy, or very high energy; each energy range seeks to investigate different aspects of hadronic;

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Progress in Neutron Star Research

Neutron stars are the collapsed cores of some massive stars. They pack roughly the mass of our Sun into a region the size of a city;

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Proceedings of the International Astronomical Union Symposia and Colloquia

IAU Symposium 303 highlights the latest Galactic Center research by scientists from around the world. Topics vary from theory through;

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Explosion Systems with Inert HighModulus Components

, which contain high modulus ceramic components. The phenomena occurring in such systems are described in detail: desensitization of high;

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Black Holes, Wormholes and Dark Energy Stars in General Relativity

of stellar configurations as the black holes, wormholes and dark energy stars.;

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From Luminous Hot Stars to Starburst Galaxies

represented by starburst phenomena. A thorough discussion of the physical and wind parameters of massive stars is presented. HII galaxies, their;

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Pulsation, Rotation and Mass Loss in Early-Type Stars

of the circumstellar envelopes around Be stars is indeed a flattened disk as they can now be optically resolved. The variability of radiatively;

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Cambridge Astrophysics

represented by starburst phenomena. A thorough discussion of the physical and wind parameters of massive stars is presented. HII galaxies, their;

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Frontiers in Organometallic Chemistry

(including light) is trapped by gravity. A black hole is an extremely compact object, collapsed by gravity which has overcome electric and nuclear;

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