Idioma: Inglés
Publicado por WSPC, 2025
Librería: Books in my Basket, New Delhi, India
EUR 24,92
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Añadir al carritoSoft cover. Condición: New. ISBN:9798886131383,pp.
Idioma: Inglés
Publicado por World Scientific (Europe), 2018
ISBN 10: 1783265809 ISBN 13: 9781783265800
Librería: GreatBookPrices, Columbia, MD, Estados Unidos de America
EUR 49,10
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Añadir al carritoCondición: New.
Idioma: Inglés
Publicado por World Scientific Publishing Europe Ltd 1/30/2019, 2019
ISBN 10: 1783265809 ISBN 13: 9781783265800
Librería: BargainBookStores, Grand Rapids, MI, Estados Unidos de America
EUR 51,47
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Añadir al carritoPaperback or Softback. Condición: New. The Structure and Evolution of Stars. Book.
Idioma: Inglés
Publicado por World Scientific (Europe), 2018
ISBN 10: 1783265809 ISBN 13: 9781783265800
Librería: California Books, Miami, FL, Estados Unidos de America
EUR 53,63
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Añadir al carritoCondición: New.
Idioma: Inglés
Publicado por Imperial College Press, GB, 2019
ISBN 10: 1783265809 ISBN 13: 9781783265800
Librería: Rarewaves.com USA, London, LONDO, Reino Unido
EUR 55,60
Cantidad disponible: 13 disponibles
Añadir al carritoPaperback. Condición: New. 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.
Idioma: Inglés
Publicado por World Scientific (Europe), 2018
ISBN 10: 1783265809 ISBN 13: 9781783265800
Librería: GreatBookPrices, Columbia, MD, Estados Unidos de America
EUR 53,89
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Añadir al carritoCondición: As New. Unread book in perfect condition.
Idioma: Inglés
Publicado por Imperial College Press, 2019
ISBN 10: 1783265809 ISBN 13: 9781783265800
Librería: PBShop.store US, Wood Dale, IL, Estados Unidos de America
EUR 57,72
Cantidad disponible: 15 disponibles
Añadir al carritoPAP. Condición: New. New Book. Shipped from UK. Established seller since 2000.
Idioma: Inglés
Publicado por Imperial College Press, GB, 2019
ISBN 10: 1783265809 ISBN 13: 9781783265800
Librería: Rarewaves USA, OSWEGO, IL, Estados Unidos de America
EUR 59,83
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Añadir al carritoPaperback. Condición: New. 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.
Idioma: Inglés
Publicado por Imperial College Press, 2019
ISBN 10: 1783265809 ISBN 13: 9781783265800
Librería: PBShop.store UK, Fairford, GLOS, Reino Unido
EUR 54,27
Cantidad disponible: 15 disponibles
Añadir al carritoPAP. Condición: New. New Book. Shipped from UK. Established seller since 2000.
Idioma: Inglés
Publicado por Imperial College Press, London, 2019
ISBN 10: 1783265809 ISBN 13: 9781783265800
Librería: Grand Eagle Retail, Bensenville, IL, Estados Unidos de America
EUR 66,86
Cantidad disponible: 1 disponibles
Añadir al carritoPaperback. Condición: new. Paperback. 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. Shipping may be from multiple locations in the US or from the UK, depending on stock availability.
Idioma: Inglés
Publicado por World Scientific (Europe), 2018
ISBN 10: 1783265809 ISBN 13: 9781783265800
Librería: GreatBookPricesUK, Woodford Green, Reino Unido
EUR 52,59
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Añadir al carritoCondición: New.
Idioma: Inglés
Publicado por World Scientific (Europe), 2018
ISBN 10: 1783265809 ISBN 13: 9781783265800
Librería: Ria Christie Collections, Uxbridge, Reino Unido
EUR 60,56
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Añadir al carritoCondición: New. In.
Idioma: Inglés
Publicado por World Scientific (Europe), 2018
ISBN 10: 1783265809 ISBN 13: 9781783265800
Librería: GreatBookPricesUK, Woodford Green, Reino Unido
EUR 59,13
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Añadir al carritoCondición: As New. Unread book in perfect condition.
Idioma: Inglés
Publicado por Imperial College Press, 2018
ISBN 10: 1783265809 ISBN 13: 9781783265800
Librería: THE SAINT BOOKSTORE, Southport, Reino Unido
EUR 58,85
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Añadir al carritoPaperback / softback. Condición: New. New copy - Usually dispatched within 4 working days.
Idioma: Inglés
Publicado por World Scientific Pub Co Inc, 2019
ISBN 10: 1783265809 ISBN 13: 9781783265800
Librería: Revaluation Books, Exeter, Reino Unido
EUR 69,90
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Añadir al carritoPaperback. Condición: Brand New. 240 pages. 9.25x6.25x1.00 inches. In Stock.
Librería: Books Puddle, New York, NY, Estados Unidos de America
EUR 84,04
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Añadir al carritoCondición: Used. 240.
EUR 82,22
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Añadir al carritoCondición: Used. 240.
EUR 81,62
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Añadir al carritoCondición: Used. 240.
Idioma: Inglés
Publicado por Imperial College Press, GB, 2019
ISBN 10: 1783265809 ISBN 13: 9781783265800
Librería: Rarewaves USA United, OSWEGO, IL, Estados Unidos de America
EUR 61,57
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Añadir al carritoPaperback. Condición: New. 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.
EUR 106,37
Cantidad disponible: 6 disponibles
Añadir al carritoCondición: New.
Idioma: Inglés
Publicado por Imperial College Press, 2019
ISBN 10: 1783265795 ISBN 13: 9781783265794
Librería: PBShop.store US, Wood Dale, IL, Estados Unidos de America
EUR 108,74
Cantidad disponible: 15 disponibles
Añadir al carritoHRD. Condición: New. New Book. Shipped from UK. Established seller since 2000.
Idioma: Inglés
Publicado por Imperial College Press, 2019
ISBN 10: 1783265795 ISBN 13: 9781783265794
Librería: PBShop.store UK, Fairford, GLOS, Reino Unido
EUR 103,30
Cantidad disponible: 15 disponibles
Añadir al carritoHRD. Condición: New. New Book. Shipped from UK. Established seller since 2000.
EUR 113,34
Cantidad disponible: 6 disponibles
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EUR 103,29
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Añadir al carritoCondición: New.
Idioma: Inglés
Publicado por Imperial College Press, GB, 2019
ISBN 10: 1783265809 ISBN 13: 9781783265800
Librería: Rarewaves.com UK, London, Reino Unido
EUR 52,58
Cantidad disponible: 13 disponibles
Añadir al carritoPaperback. Condición: New. 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.
EUR 115,50
Cantidad disponible: 12 disponibles
Añadir al carritoCondición: New. In.
EUR 113,79
Cantidad disponible: 6 disponibles
Añadir al carritoCondición: As New. Unread book in perfect condition.
Idioma: Inglés
Publicado por Imperial College Press, 2018
ISBN 10: 1783265795 ISBN 13: 9781783265794
Librería: THE SAINT BOOKSTORE, Southport, Reino Unido
EUR 114,49
Cantidad disponible: 6 disponibles
Añadir al carritoHardback. Condición: New. New copy - Usually dispatched within 4 working days.
Idioma: Inglés
Publicado por Imperial College Press, London, 2019
ISBN 10: 1783265809 ISBN 13: 9781783265800
Librería: AussieBookSeller, Truganina, VIC, Australia
EUR 102,02
Cantidad disponible: 1 disponibles
Añadir al carritoPaperback. Condición: new. Paperback. 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. Shipping may be from our Sydney, NSW warehouse or from our UK or US warehouse, depending on stock availability.
Idioma: Inglés
Publicado por World Scientific Pub Co Inc, 2019
ISBN 10: 1783265795 ISBN 13: 9781783265794
Librería: Revaluation Books, Exeter, Reino Unido
EUR 138,90
Cantidad disponible: 2 disponibles
Añadir al carritoHardcover. Condición: Brand New. 338 pages. 9.25x6.25x1.00 inches. In Stock.