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140122 ||| eng |
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|a 9781447100591
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|a Inglis, Mike
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| 245 |
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|a Observer’s Guide to Stellar Evolution
|h Elektronische Ressource
|b The Birth, Life and Death of Stars
|c by Mike Inglis
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| 250 |
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|a 1st ed. 2003
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| 260 |
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|a London
|b Springer London
|c 2003, 2003
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| 300 |
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|a XVII, 238 p
|b online resource
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|a 3.3 From the Surface to the Core -- 3.4 The Proton—Proton Chain -- 3.5 The Flow of Energy from the Core to the Surface -- 3.6 Main Sequence Lifetimes -- 3.7 Towards the Red Giant -- 3.8 Helium Burning and the Helium Flash -- 3.9 Red Giants, Star Clusters and the H—R Diagram -- 3.10 Post-Main Sequence Star Clusters: The Globular Clusters -- 3.11 Stars That Pulsate -- 3.12 Cepheid Variables and the Period—Luminosity Relationship -- 3.13 Cepheid Variables: Temperature and Mass -- 3.14 RR Lyrae and Long-Period Variable Stars -- 4 The End Point — Star Death -- 4.1 Introduction -- 4.2 The Asymptotic Giant Branch -- 4.3 Dredge-Ups -- 4.4 Mass Loss and Stellar Winds -- 4.5 Infrared Stars -- 4.6 The End of an AGB Star’s Life -- 4.7 Planetary Nebulae -- 4.8 White Dwarf Stars -- 4.9 Electron Degeneracy and White Dwarfs -- 4.10 The Chandrasekhar Limit -- 4.11 WhiteDwarf Evolution -- 4.12 White Dwarf Origins -- 4.13 High-Mass Stars: Nuclear Burning and an Onion --
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|a 4.14 Iron, Supernovae and the Formation of the Elements -- 4.15 The Supernova Remnant -- 4.16 A Final Note on Supernovae -- 4.17 Neutron Stars, Pulsars and Black Holes -- 4.18 From Beginning to End -- Appendix 1 Degeneracy -- Appendix 2 Books, Magazines and Organizations -- Appendix 3 The Greek Alphabet -- Appendix 4 Colour Photographs -- Object Index
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|a A Brief Introduction -- 1 Stellar Evolution — The Basics -- 1.1 Distance to the Stars -- 1.2 The Nearest Stars -- 1.3 The Brightness and Luminosity of Stars -- 1.4 The Magnitudes of Stars -- 1.5 The Brightest Stars -- 1.6 The Colour of Stars -- 1.7 The Size and Mass of Stars -- 1.8 The Biggest Stars -- 1.9 The Constituents of Stars -- 1.10 The Spectra of Stars -- 1.11 Stellar Classification -- 1.12 The Hertzsprung—Russell Diagram -- 1.13 The H—R Diagram and a Star’s Radius -- 1.14 The H—R Diagram and a Star’s Luminosity -- 1.15 The H—R Diagram and a Star’s Mass -- 2 Beginnings — Star Birth -- 2.1 Introduction -- 2.2 The Interstellar Medium -- 2.3 Nebulae -- 2.4 Molecular Clouds -- 2.5 Protostars -- 2.6 Pre-Main Sequence Evolution -- 2.7 Mass Loss and Mass Gain -- 2.8 Star Clusters -- 2.9 Stellar Associations and Streams -- 2.10 Star Formation Triggers -- 3 The Main Sequence and Beyond -- 3.1 Introduction -- 3.2 Our Nearest Star — The Sun --
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| 653 |
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|a Astronomy / Observations
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| 653 |
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|a Astronomy, Observations and Techniques
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| 041 |
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|a eng
|2 ISO 639-2
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| 989 |
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|b SBA
|a Springer Book Archives -2004
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| 490 |
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|a The Patrick Moore Practical Astronomy Series
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|a 10.1007/978-1-4471-0059-1
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| 856 |
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|u https://doi.org/10.1007/978-1-4471-0059-1?nosfx=y
|x Verlag
|3 Volltext
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|a 520
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|a Stellar evolution - the birth, development and death of stars - is central to our current understanding of astronomy. This area of astrophysics is often portrayed as being difficult and mathematical, but Mike Inglis brings it to life in a unique way, combining a step-by-step introduction with suggestions for making practical observations of stars at different stages in their evolution. Every amateur astronomer - regardless of their current level of knowledge - will find this book fascinating and informative
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