Structure and Evolution of Stars, Paperback by Eldridge, J. J.; Tout, Christo...
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Structure and Evolution of Stars, Paperback by Eldridge, J. J.; Tout, Christo...
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N.º de artículo de eBay:388332115568
Última actualización el 15 jul 2025 05:55:46 H.EspVer todas las actualizacionesVer todas las actualizaciones
Características del artículo
- Estado
- ISBN
- 9781783265800
Acerca de este producto
Product Identifiers
Publisher
Imperial College Press
ISBN-10
1783265809
ISBN-13
9781783265800
eBay Product ID (ePID)
234846931
Product Key Features
Book Title
Structure and Evolution of Stars
Topic
Physics / Quantum Theory, Physics / Nuclear, Astronomy
Publication Year
2017
Number of Pages
240 Pages
Language
English
Illustrator
Yes
Genre
Science
Format
Trade Paperback
Additional Product Features
Intended Audience
Trade
LCCN
2018-033728
TitleLeading
The
Dewey Edition
23
Dewey Decimal
523.88
Synopsis
Stars are the fundamental observable constituents of the Universe. They are the first objects we see in the night sky, they dominate the light produced in our own and other galaxies, and nucleosynthesis in stars produces all the elements heavier than helium. A knowledge of stars and their evolution is vital to understand other astrophysical objects from accreting black holes and galaxies to the Universe itself.The structure of a star can be described mathematically by differential equations derived from the principles of hydrodynamics, electromagnetic theory, thermodynamics, quantum mechanics, atomic and nuclear physics. The basic equations of a spherical star are derived in detail at an accessible level. The topics discussed include modes of energy transport, the equation of state, the physics of the opacity sources and the nuclear reactions. Attention is also given to the virial theorem, polytropic gas spheres and homology principles and the procedure for numerical solution of the equations is outlined. This book tracks the evolution of stars from their main-sequence evolution through the exhaustion of various nuclear fuels to the end points of evolution and also introduces the topic of interacting binary stars. The aim is to take the reader from the essential underlying physical principles to the doors to current research on stellar interiors., Stars are the fundamental observable constituents of the Universe. They are the first objects we see in the night sky, they dominate the light produced in our own and other galaxies, and nucleosynthesis in stars produces all the elements heavier than helium. A knowledge of stars and their evolution is vital to understand other astrophysical objects from accreting black holes and galaxies to the Universe itself. The structure of a star can be described mathematically by differential equations derived from the principles of hydrodynamics, electromagnetic theory, thermodynamics, quantum mechanics, atomic and nuclear physics. The basic equations of a spherical star are derived in detail at an accessible level. The topics discussed include modes of energy transport, the equation of state, the physics of the opacity sources and the nuclear reactions. Attention is also given to the virial theorem, polytropic gas spheres and homology principles and the procedure for numerical solution of the equations is outlined. This book tracks the evolution of stars from their main-sequence evolution through the exhaustion of various nuclear fuels to the end points of evolution and also introduces the topic of interacting binary stars. The aim is to take the reader from the essential underlying physical principles to the doors to current research on stellar interiors., Stars are the fundamental observable constituents of the Universe. They are the first objects we see in the night sky, dominate the light produced in our own and other galaxies and nucleosynthesis in stars produces all the elements heavier than helium. A knowledge of stars and their evolution is vital in understanding other astrophysical objects from accreting black holes and galaxies to the Universe itself.The structure of a star can be described mathematically by differential equations which can be derived from the principles of hydrodynamics, electromagnetic theory, thermodynamics, quantum mechanics, and atomic and nuclear physics. The basic equations of a spherical star are derived in detail, the modes of energy transport, the equation of state, the physics of the opacity sources and the nuclear reactions are explained. Approximate solutions of the equations for stellar structure are given. Attention is given to the virial theorem, polytropic gas spheres and homology principles. The procedure for numerical solution of the equations is outlined.The evolution of a star is described from its main sequence evolution through the exhaustion of various nuclear fuels to the end points of evolution such as white dwarfs, neutron stars and black holes. Supernova explosions as the deaths of massive stars along with the nucleosynthesis of elements within stars are explained.
LC Classification Number
QB806.E53 2018
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- l***1 (1485)- Votos emitidos por el comprador.Últimos 6 mesesCompra verificadaGreat seller; book exactly as described in mint condition sold at a reasonable price; seller shipped item FAST, FREE and with tracking information, a must nowadays; seller shipped in tight, cardboard mailing envelope, which tightly fit over the book, preventing damage in shipment; good communication too; rate seller 10+++++Cuentos de La Habana Elegante, Brand New, Free shipping in the US (#364594098367)
- y***t (1862)- Votos emitidos por el comprador.Últimos 6 mesesCompra verificadaI purchase the Veterinary Assisting Fundamentals & Applications, Hardcover by Vanhorn, Beth on January 22nd and it took five days which was January 27th to confirm my order, provide a tracking . Once, that happend the textbook sat somewhere 4 more days before it was shipped , it was suppose to arrive Monday, January 3rd, Great seller. Great price, As described, Packed well.Veterinary Assisting Fundamentals & Applications, Hardcover by Vanhorn, Beth,... (#384492381860)