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Uspekhi Fizicheskih Nauk, 1964
CONTENTS 1. Introduction 763 2. Equilibrium and Stability of a Star as a Whole 764 3. Equation of State 767 4. Masses of Stars in the Final Stages of Evolution 769 5. Schwarzschild Gravitation Field 770 6. Gravitational Field Inside a Star 771 7. Paths of Light Rays Inside and Outside a Static Star 772 8. Structure of Superdense Stars 773 9.
Ya B Zel'dovich, Igor D Novikov
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CONTENTS 1. Introduction 763 2. Equilibrium and Stability of a Star as a Whole 764 3. Equation of State 767 4. Masses of Stars in the Final Stages of Evolution 769 5. Schwarzschild Gravitation Field 770 6. Gravitational Field Inside a Star 771 7. Paths of Light Rays Inside and Outside a Static Star 772 8. Structure of Superdense Stars 773 9.
Ya B Zel'dovich, Igor D Novikov
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2008 22nd International Symposium on High Performance Computing Systems and Applications, 2008
Summary form only given. Large-scale computation has achieved a pivotal role in many areas of astrophysics and cosmology. Not only does increasing computational power allow us to better model the huge range of spatial and temporal scales in the universe, but simulations provide in many cases the only laboratory in which we may actively experiment on ...
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Summary form only given. Large-scale computation has achieved a pivotal role in many areas of astrophysics and cosmology. Not only does increasing computational power allow us to better model the huge range of spatial and temporal scales in the universe, but simulations provide in many cases the only laboratory in which we may actively experiment on ...
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The astrophysics of crowded places
Philosophical Transactions of the Royal Society of London. Series A: Mathematical, Physical and Engineering Sciences, 2002Today the Sun is in a relatively uncrowded place. The distance between it and the nearest other star is relatively large (about 200,000 times the Earth-Sun distance!). This is beneficial to life on Earth; a close encounter with another star is extremely unlikely. Such encounters would either remove the Earth from its orbit around the Sun or leave it on
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